Author: "Gatti M." / Database: OpenAIRE - Searchworks@Jio Institute Digital Library Search Results

Your search keyword '"Gatti M."' showing total 389 results

Start Over Author "Gatti M." Database OpenAIRE

389 results on '"Gatti M."'

1. Constraining the baryonic feedback with cosmic shear using the DES Year-3 small-scale measurements

Author: Chen, A., Aricò, G., Huterer, D., Angulo, R. E., Weaverdyck, N., Friedrich, O., Secco, L. F., Hernández-Monteagudo, C., Alarcon, A., Alves, O., Amon, A., Andrade-Oliveira, F., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Blazek, J., Brandao-Souza, A., Bridle, S. L., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Chang, C., Chen, R., Chintalapati, P., Choi, A., Cordero, J., Crocce, M., Pereira, M. E. S., Davis, C., Derose, J., Di Valentino, E., Diehl, H. T., Dodelson, S., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Elvin-Poole, J., Everett, S., Fang, X., Ferté, A., Fosalba, P., Gatti, M., Gaztanaga, E., Giannini, G., Gruen, D., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Hoffmann, K., Huang, H., Huff, E. M., Jain, B., Jarvis, M., Jeffrey, N., Kacprzak, T., Krause, E., Kuropatkin, N., Leget, P. -F., Lemos, P., Liddle, A. R., Maccrann, N., Mccullough, J., Muir, J., Myles, J., Navarro-Alsina, A., Omori, Y., Pandey, S., Park, Y., Porredon, A., Prat, J., Raveri, M., Refregier, A., Rollins, R. P., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, J., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troja, A., Troxel, M. A., Tutusaus, I., Varga, T. N., Wechsler, R. H., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Aguena, M., Annis, J., Bacon, D., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Carretero, J., Conselice, C., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Paz-Chinchón, F., Pieres, A., Sanchez, E., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Des, Collaboration, Chen, A., Aricò, G., Huterer, D., Angulo, R. E., Weaverdyck, N., Friedrich, O., Secco, L. F., Hernández-Monteagudo, C., Alarcon, A., Alves, O., Amon, A., Andrade-Oliveira, F., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Blazek, J., Brandao-Souza, A., Bridle, S. L., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Chang, C., Chen, R., Chintalapati, P., Choi, A., Cordero, J., Crocce, M., Pereira, M. E. S., Davis, C., Derose, J., Di Valentino, E., Diehl, H. T., Dodelson, S., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Elvin-Poole, J., Everett, S., Fang, X., Ferté, A., Fosalba, P., Gatti, M., Gaztanaga, E., Giannini, G., Gruen, D., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Hoffmann, K., Huang, H., Huff, E. M., Jain, B., Jarvis, M., Jeffrey, N., Kacprzak, T., Krause, E., Kuropatkin, N., Leget, P. -F., Lemos, P., Liddle, A. R., Maccrann, N., Mccullough, J., Muir, J., Myles, J., Navarro-Alsina, A., Omori, Y., Pandey, S., Park, Y., Porredon, A., Prat, J., Raveri, M., Refregier, A., Rollins, R. P., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, J., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troja, A., Troxel, M. A., Tutusaus, I., Varga, T. N., Wechsler, R. H., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Aguena, M., Annis, J., Bacon, D., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Carretero, J., Conselice, C., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Paz-Chinchón, F., Pieres, A., Sanchez, E., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., and Des, Collaboration
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Nuclear Theory, High Energy Physics::Phenomenology, cosmology observations, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics Cosmology and Nongalactic Astrophysics, Space and Planetary Science, gravitational lensing weak, large-scale structure of Universe, cosmology observation, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We use the small scales of the Dark Energy Survey (DES) Year-3 cosmic shear measurements, which are excluded from the DES Year-3 cosmological analysis, to constrain the baryonic feedback. To model the baryonic feedback, we adopt a baryonic correction model and use the numerical package \texttt{Baccoemu} to accelerate the evaluation of the baryonic nonlinear matter power spectrum. We design our analysis pipeline to focus on the constraints of the baryonic suppression effects, utilizing the implication given by a principal component analysis on the Fisher forecasts. Our constraint on the baryonic effects can then be used to better model and ameliorate the effects of baryons in producing cosmological constraints from the next generation large-scale structure surveys. We detect the baryonic suppression on the cosmic shear measurements with a $\sim 2 \sigma$ significance. The characteristic halo mass for which half of the gas is ejected by baryonic feedback is constrained to be $M_c > 10^{13.2} h^{-1} M_{\odot}$ (95\% C.L.). The best-fit baryonic suppression is $\sim 5\%$ at $k=1.0 {\rm Mpc}\ h^{-1}$ and $\sim 15\%$ at $k=5.0 {\rm Mpc} \ h^{-1}$. Our findings are robust with respect to the assumptions about the cosmological parameters, specifics of the baryonic model, and intrinsic alignments., Comment: 20 pages, 10 figures. DES Collaboration, Year-3 analysis
Published: 2022

2. Non-local contribution from small scales in galaxy–galaxy lensing: comparison of mitigation schemes

Author: Prat, J., Zacharegkas, G., Park, Y., MacCrann, N., Switzer, E. R., Pandey, S., Chang, C., Blazek, J., Miquel, R., Alarcon, A., Alves, O., Amon, A., Andrade-Oliveira, F., Bechtol, K., Becker, M. R., Bernstein, G. M., Chen, R., Choi, A., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Cordero, J., Crocce, M., Davis, C., DeRose, J., Diehl, H. T., Dodelson, S., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elvin-Poole, J., Everett, S., Fang, X., Ferté, A., Fosalba, P., Friedrich, O., Gatti, M., Giannini, G., Gruen, D., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Huang, H., Huff, E. M., Jarvis, M., Krause, E., Kuropatkin, N., Leget, P.-F., McCullough, J., Myles, J., Navarro-Alsina, A., Porredon, A., Raveri, M., Rollins, R. P., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Sánchez, C., Sanchez, J., Secco, L. F., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troxel, M. A., Tutusaus, I., Varga, T. N., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Carretero, J., Costanzi, M., Pereira, M. E. S., De Vicente, J., Desai, S., Ferrero, I., Flaugher, B., Gerdes, D. W., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Lima, M., Menanteau, F., Mena-Fernández, J., Palmese, A., Paterno, M., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A. A., Rodriguez-Monroy, M., Sanchez, E., Schubnell, M., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., To, C., Weaverdyck, N., and Weller, J.
Abstract: Recent cosmological analyses with large-scale structure and weak lensing measurements, usually referred to as 3 × 2pt, had to discard a lot of signal to noise from small scales due to our inability to accurately model non-linearities and baryonic effects. Galaxy–galaxy lensing, or the position–shear correlation between lens and source galaxies, is one of the three two-point correlation functions that are included in such analyses, usually estimated with the mean tangential shear. However, tangential shear measurements at a given angular scale θ or physical scale R carry information from all scales below that, forcing the scale cuts applied in real data to be significantly larger than the scale at which theoretical uncertainties become problematic. Recently, there have been a few independent efforts that aim to mitigate the non-locality of the galaxy–galaxy lensing signal. Here, we perform a comparison of the different methods, including the Y-transformation, the point-mass marginalization methodology, and the annular differential surface density statistic. We do the comparison at the cosmological constraints level in a combined galaxy clustering and galaxy–galaxy lensing analysis. We find that all the estimators yield equivalent cosmological results assuming a simulated Rubin Observatory Legacy Survey of Space and Time (LSST) Year 1 like set-up and also when applied to DES Y3 data. With the LSST Y1 set-up, we find that the mitigation schemes yield ∼1.3 times more constraining S8 results than applying larger scale cuts without using any mitigation scheme.
Published: 2023

3. The DES view of the Eridanus supervoid and the CMB cold spot

Author: Kovács, A, Jeffrey, N, Gatti, M, Chang, C, Whiteway, L, Hamaus, N, Lahav, O, Pollina, G, Bacon, D, Kacprzak, T, Mawdsley, B, Nadathur, S, Zeurcher, D, García-Bellido, J, Alarcon, A, Amon, A, Bechtol, K, Bernstein, G M, Campos, A, Rosell, A Carnero, Kind, M Carrasco, Cawthon, R, Chen, R, Choi, A, Cordero, J, Davis, C, Derose, J, Doux, C, Drlica-Wagner, A, Eckert, K, Elsner, F, Elvin-Poole, J, Everett, S, Ferté, A, Giannini, G, Gruen, D, Gruendl, R A, Harrison, I, Hartley, W G, Herner, K, Huff, E M, Huterer, D, Kuropatkin, N, Jarvis, M, Leget, P F, Maccrann, N, Mccullough, J, Muir, J, Myles, J, Navarro-Alsina, A, Pandey, S, Prat, J, Raveri, M, Rollins, R P, Ross, A J, Rykoff, E S, Sánchez, C, Secco, L F, Sevilla-Noarbe, I, Sheldon, E, Shin, T, Troxel, M A, Tutusaus, I, Varga, T N, Yanny, B, Yin, B, Zhang, Y, Zuntz, J, Aguena, M, Allam, S, Andrade-Oliveira, F, Annis, J, Bertin, E, Brooks, D, Burke, D, Carretero, J, Costanzi, M, da&nbsp, Costa, L N, Pereira, M E S, Davis, T, Deundefined, Vicente, J, Desai, S, Diehl, H T, Ferrero, I, Flaugher, B, Fosalba, P, Frieman, J, Gaztañaga, E, Gerdes, D, Giannantonio, T, Gschwend, J, Gutierrez, G, Hinton, S, Hollowood, D L, Honscheid, K, James, D, Kuehn, K, Lima, M, Maia, M A G, Marshall, J L, Melchior, P, Menanteau, F, Miquel, R, Morgan, R, Ogando, R, Paz-Chinchon, F, Pieres, A, Plazas, A A, Monroy, M Rodriguez, Romer, K, Roodman, A, Sanchez, E, Schubnell, M, Serrano, S, Smith, M, Soares-Santos, M, Suchyta, E, Swanson, M E C, Tarle, G, Thomas, D, C-H, To, Weller, J, UAM. Departamento de Física Teórica, Instituto de Astrofísica de Canarias (IAC), Tenerife, Univer Sité de Paris, University College London, The Barcelona Institute of Science and Technology, University of Pennsylvania, University of Chicago, Univer Sity of Chica Go, Ludwig-Maximilians Univer- Sität München, University of Portsmouth, ETH Zurich, Universidad Autonoma de Madrid, Argonne National Laboratory, Stanford University, University of Wisconsin- Madison, Carnegie Mellon University, Laboratório Interinstitucional de E-Astronomia - LIneA, National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign, Duke University, The Ohio State Univer- Sity, University of Manchester, University of California, Santa Cruz Institute for Particle Physics, Fermi National Accelerator Laboratory, The Ohio State University, California Institute of Technology, SLAC National Accelerator Laboratory, University of Oxford, University of Gene Va, University of Michigan, University of Cambridge, Perimeter Institute for Theoretical Physics, Univer Sidade Estadual de Campinas, Medioambientales y Tecnológicas (CIEMAT), Brookhaven National Laboratory, Institut D'Estudis Espacials de Catalunya (IEEC), CSIC), Max Planck Institute for Extraterrestrial Physics, University of Edinb Urgh, Universidade de São Paulo (USP), Universidade Estadual Paulista (UNESP), Institut D'Astrophysique de Paris, University of Trieste, INAF-Osservatorio Astronomico di Trieste, Institute for Fundamental Physics of the Universe, Observatório Nacional, University of Queensland, IIT Hyderabad, University of Oslo, Univer Sity of Cambridge, Harvard and Smithsonian, Lowell Observatory, Macquarie University, Texas A&M Univer Sity, Princeton University, Institució Catalana de Recerca i Estudis Avan C Ats, Univer Sity of Sussex, University of Southampton, Oak Ridge National Labo- Ratory, Kovács, A, Jeffrey, N, Gatti, M, Chang, C, Whiteway, L, Hamaus, N, Lahav, O, Pollina, G, Bacon, D, Kacprzak, T, Mawdsley, B, Nadathur, S, Zeurcher, D, García-Bellido, J, Alarcon, A, Amon, A, Bechtol, K, Bernstein, G M, Campos, A, Rosell, A Carnero, Kind, M Carrasco, Cawthon, R, Chen, R, Choi, A, Cordero, J, Davis, C, Derose, J, Doux, C, Drlica-Wagner, A, Eckert, K, Elsner, F, Elvin-Poole, J, Everett, S, Ferté, A, Giannini, G, Gruen, D, Gruendl, R A, Harrison, I, Hartley, W G, Herner, K, Huff, E M, Huterer, D, Kuropatkin, N, Jarvis, M, Leget, P F, Maccrann, N, Mccullough, J, Muir, J, Myles, J, Navarro-Alsina, A, Pandey, S, Prat, J, Raveri, M, Rollins, R P, Ross, A J, Rykoff, E S, Sánchez, C, Secco, L F, Sevilla-Noarbe, I, Sheldon, E, Shin, T, Troxel, M A, Tutusaus, I, Varga, T N, Yanny, B, Yin, B, Zhang, Y, Zuntz, J, Aguena, M, Allam, S, Andrade-Oliveira, F, Annis, J, Bertin, E, Brooks, D, Burke, D, Carretero, J, Costanzi, M, da&nbsp, Costa, L N, Pereira, M E S, Davis, T, De&nbsp, Vicente, J, Desai, S, Diehl, H T, Ferrero, I, Flaugher, B, Fosalba, P, Frieman, J, Gaztañaga, E, Gerdes, D, Giannantonio, T, Gschwend, J, Gutierrez, G, Hinton, S, Hollowood, D L, Honscheid, K, James, D, Kuehn, K, Lima, M, Maia, M A G, Marshall, J L, Melchior, P, Menanteau, F, Miquel, R, Morgan, R, Ogando, R, Paz-Chinchon, F, Pieres, A, Plazas, A A, Monroy, M Rodriguez, Romer, K, Roodman, A, Sanchez, E, Schubnell, M, Serrano, S, Smith, M, Soares-Santos, M, Suchyta, E, Swanson, M E C, Tarle, G, Thomas, D, C-H, To, Weller, J, Ministerio de Ciencia, Innovación y Universidades (España), Agencia Estatal de Investigación (España), Ministerio de Economía y Competitividad (España), European Research Council, National Science Foundation (US), European Commission, and Agenzia Spaziale Italiana
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cosmic Background Radiation, FOS: Physical sciences, Física, Astronomy and Astrophysics, cosmic background radiation, Surveys, gravitational lensing: weak, surveys, Space and Planetary Science, Weak [Gravitational Lensing], survey, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: A. Kovács et al., The Cold Spot is a puzzling large-scale feature in the Cosmic Microwave Background temperature maps and its origin has been subject to active debate. As an important foreground structure at low redshift, the Eridanus supervoid was recently detected, but it was subsequently determined that, assuming the standard ΛCDM model, only about 10–20 per cent of the observed temperature depression can be accounted for via its Integrated Sachs–Wolfe imprint. However, R ≳ 100 h−1Mpc supervoids elsewhere in the sky have shown ISW imprints AISW ≈ 5.2 ± 1.6 times stronger than expected from ΛCDM (AISW = 1), which warrants further inspection. Using the Year-3 redMaGiC catalogue of luminous red galaxies from the Dark Energy Survey, here we confirm the detection of the Eridanus supervoid as a significant underdensity in the Cold Spot’s direction at z < 0.2. We also show, with S/N ≳ 5 significance, that the Eridanus supervoid appears as the most prominent large-scale underdensity in the dark matter mass maps that we reconstructed from DES Year-3 gravitational lensing data. While we report no significant anomalies, an interesting aspect is that the amplitude of the lensing signal from the Eridanus supervoid at the Cold Spot centre is about 30 per cent lower than expected from similar peaks found in N-body simulations based on the standard ΛCDM model with parameters Ωm = 0.279 and σ8 = 0.82. Overall, our results confirm the causal relation between these individually rare structures in the cosmic web and in the CMB, motivating more detailed future surveys in the Cold Spot region., AK has been supported by a Juan de la Cierva Incorporación fellowship with project number IJC2018-037730-I, and funding for this project was also available in part through SEV-2015-0548 and AYA2017-89891-P. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The DES data management system is supported by the National Science Foundation under Grant Numbers AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under grants ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq grant 465376/2014-2).
Published: 2021

4. Mapping Variations of Redshift Distributions with Probability Integral Transforms

Author: Myles, J., Gruen, D., Amon, A., Alarcon, A., DeRose, J., Everett, S., Dodelson, S., Bernstein, G. M., Campos, A., Harrison, I., MacCrann, N., McCullough, J., Raveri, M., Sánchez, C., Troxel, M. A., Yin, B., Abbott, T. M. C., Allam, S., Alves, O., Andrade-Oliveira, F., Bertin, E., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cawthon, R., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Desai, S., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gatti, M., Gerdes, D. W., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., Melchior, P., Mena-Fernández, J., Menanteau, F., Miquel, R., Mohr, J. J., Palmese, A., Paz-Chinchón, F., Pieres, A., Malagón, A. A. Plazas, Prat, J., Rodriguez-Monroy, M., Sanchez, E., Scarpine, V., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Tucker, D. L., Vincenzi, M., Weaverdyck, N., DES Collaboration, Myles, J., Gruen, D., Amon, A., Alarcon, A., Derose, J., Everett, S., Dodelson, S., Bernstein, G. M., Campos, A., Harrison, I., Maccrann, N., Mccullough, J., Raveri, M., Sánchez, C., Troxel, M. A., Yin, B., Abbott, T. M. C., Allam, S., Alves, O., Andrade-Oliveira, F., Bertin, E., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cawthon, R., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Desai, S., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gatti, M., Gerdes, D. W., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., Melchior, P., Mena-Fernández, J., Menanteau, F., Miquel, R., Mohr, J. J., Palmese, A., Paz-Chinchón, F., Pieres, A., Malagón, A. A. Plaza, Prat, J., Rodriguez-Monroy, M., Sanchez, E., Scarpine, V., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Tucker, D. L., Vincenzi, M., Weaverdyck, N., and Des, Collaboration
Subjects: Astrophysic, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Space and Planetary Science, galaxies distances and redshift, FOS: Physical sciences, Astronomy and Astrophysics, gravitational lensing weak, methods numerical, galaxies distances and redshifts, Astrophysics, Cosmology and Nongalactic Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present a method for mapping variations between probability distribution functions and apply this method within the context of measuring galaxy redshift distributions from imaging survey data. This method, which we name PITPZ for the probability integral transformations it relies on, uses a difference in curves between distribution functions in an ensemble as a transformation to apply to another distribution function, thus transferring the variation in the ensemble to the latter distribution function. This procedure is broadly applicable to the problem of uncertainty propagation. In the context of redshift distributions, for example, the uncertainty contribution due to certain effects can be studied effectively only in simulations, thus necessitating a transfer of variation measured in simulations to the redshift distributions measured from data. We illustrate the use of PITPZ by using the method to propagate photometric calibration uncertainty to redshift distributions of the Dark Energy Survey Year 3 weak lensing source galaxies. For this test case, we find that PITPZ yields a lensing amplitude uncertainty estimate due to photometric calibration error within 1 per cent of the truth, compared to as much as a 30 per cent underestimate when using traditional methods.
Published: 2022

5. Dark Energy Survey Year 3 results: Cosmology from combined galaxy clustering and lensing validation on cosmological simulations

Author: DeRose, J., Wechsler, R. H., Becker, M. R., Rykoff, E. S., Pandey, S., MacCrann, N., Amon, A., Myles, J., Krause, E., Gruen, D., Jain, B., Troxel, M. A., Prat, J., Alarcon, A., Sanchez, C., Blazek, J., Crocce, M., Giannini, G., Gatti, M., Bernstein, G. M., Zuntz, J., Dodelson, S., Fang, X., Friedrich, O., Secco, L. F., Elvin-Poole, J., Porredon, A., Everett, S., Choi, A., Harrison, I., Cordero, J., Rodriguez-Monroy, M., McCullough, J., Cawthon, R., Chen, A., Alves, O., Andrade-Oliveira, F., Bechtol, K., Camacho, H., Campos, A., Rosell, A. Carnero, Kind, M. Carrasco, Diehl, H. T., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Gruendl, R. A., Hartley, W. G., Huang, H., Huff, E. M., Kuropatkin, N., Raveri, M., Rosenfeld, R., Ross, A. J., Sanchez, J., Sevilla-Noarbe, I., Sheldon, E., Yanny, B., Yin, B., Zhang, Y., Fosalba, P., Aguena, M., Allam, S., Annis, J., Avila, S., Bacon, D., Bhargava, S., Brooks, D., Buckley-Geer, E., Burke, D. L., Carretero, J., Castander, F. J., Chang, C., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Evrard, A. E., Ferrero, I., Ferte, A., Flaugher, B., Frieman, J., Garcia-Bellido, J., Gaztanaga, E., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Huterer, D., James, D. J., Kuehn, K., Lahav, O., Lima, M., Maia, M. A. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Palmese, A., Paz-Chinchon, F., Petravick, D., Pieres, A., Malagon, A. A. Plazas, Sanchez, E., Scarpine, V., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., UAM. Departamento de Física Teórica, A DeRose, J., Wechsler, R. H., Becker, M. R., Rykoff, E. S., Pandey, S., Maccrann, N., Amon, A., Myles, J., Krause, E., Gruen, D., Jain, B., Troxel, M. A., Prat, J., Alarcon, A., Sánchez, C., Blazek, J., Crocce, M., Giannini, G., Gatti, M., Bernstein, G. M., Zuntz, J., Dodelson, S., Fang, X., Friedrich, O., Secco, L. F., Elvin-Poole, J., Porredon, A., Everett, S., Choi, A., Harrison, I., Cordero, J., Rodriguez-Monroy, M., Mccullough, J., Cawthon, R., Chen, A., Alves, O., Andrade-Oliveira, F., Bechtol, K., Camacho, H., Campos, A., Rosell, A. Carnero, Kind, M. Carrasco, Diehl, H. T., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Gruendl, R. A., Hartley, W. G., Huang, H., Huff, E. M., Kuropatkin, N., Raveri, M., Rosenfeld, R., Ross, A. J., Sanchez, J., Sevilla-Noarbe, I., Sheldon, E., Yanny, B., Yin, B., Zhang, Y., Fosalba, P., Aguena, M., Allam, S., Annis, J., Avila, S., Bacon, D., Bhargava, S., Brooks, D., Buckley-Geer, E., Burke, D. L., Carretero, J., Castander, F. J., Chang, C., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Evrard, A. E., Ferrero, I., Ferté, A., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Huterer, D., James, D. J., Kuehn, K., Lahav, O., Lima, M., Maia, M. A. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Palmese, A., Paz-Chinchón, F., Petravick, D., Pieres, A., Malagón, A. A. Plaza, Sanchez, E., Scarpine, V., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., Department of Energy (US), National Science Foundation (US), Ministerio de Ciencia, Innovación y Universidades (España), Agencia Estatal de Investigación (España), Ministerio de Economía y Competitividad (España), European Commission, European Research Council, and Generalitat de Catalunya
Subjects: data release, Gravitational Lensing, model, Cosmology and Nongalactic Astrophysics (astro-ph.CO), sky surveys, strophysics, FOS: Physical sciences, Física, Astrophysics::Cosmology and Extragalactic Astrophysics, oscillation spectroscopic survey, calibration, des, Dark Energy, Cosmology and Nongalactic Astrophysics, strophysic, challenge, impact, astro-ph.CO, Weak, redshift distributions, sdss, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: J. DeRose et al., We present a validation of the Dark Energy Survey Year 3 (DES Y3) 3×2-point analysis choices by testing them on Buzzard2.0, a new suite of cosmological simulations that is tailored for the testing and validation of combined galaxy clustering and weak-lensing analyses. We show that the buzzard2.0 simulations accurately reproduce many important aspects of the DES Y3 data, including photometric redshift and magnitude distributions, and the relevant set of two-point clustering and weak-lensing statistics. We then show that our model for the 3×2-point data vector is accurate enough to recover the true cosmology in simulated surveys assuming the true redshift distributions for our source and lens samples, demonstrating robustness to uncertainties in the modeling of the nonlinear matter power spectrum, nonlinear galaxy bias, and higher-order lensing corrections. Additionally, we demonstrate for the first time that our photometric redshift calibration methodology, including information from photometry, spectroscopy, clustering cross-correlations, and galaxy–galaxy lensing ratios, is accurate enough to recover the true cosmology in simulated surveys in the presence of realistic photometric redshift uncertainties., J. D. is supported by the Chamberlain fellowship at Lawrence Berkeley National Laboratory. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility located at Lawrence Berkeley National Laboratory, operated under Contract No. DE-AC02-05CH11231. We would like to thank Stanford University and the Stanford Research Computing Center for providing computational resources and support that contributed to these research results. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministerio da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DESBrazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciencies de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the LudwigMaximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, NFS’s NOIRLab, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. This paper is based in part on observations at Cerro Tololo Inter-American Observatory at NSF’s NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under Grants No. AST1138766andNo.AST-1536171.The DES participants from Spanish institutions are partially supported by MICINN under Grants No. ESP2017-89838, No. PGC2018094773, No. PGC2018-102021, No. SEV-2016-0588, No. SEV-2016-0597, and No. MDM-2015-0509, some of which include ERDF funds from the European Union. I.F. A.E. is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (Grant No. FP7/2007-2013) including ERC Grants No. 240672, No.291329,andNo.306478.Weacknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia(INCT)doe-Universo(CNPqGrantNo.465376/ 2014-2). This manuscript has been authored by Fermi Research Alliance, LLC, under Contract No. DE-AC0207CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics.
Published: 2022

6. Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-$y$-maps from SPT and Planck

Author: Sánchez, J., Omori, Y., Chang, C., Bleem, L. E., Crawford, T., Drlica-Wagner, A., Raghunathan, S., Zacharegkas, G., Abbott, T. M. C., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Avila, S., Baxter, E., Bechtol, K., Benson, B. A., Bernstein, G. M., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Campos, A., Carlstrom, J. E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F. J., Cawthon, R., Chang, C. L., Chen, A., Choi, A., Chown, R., Costanzi, M., Crites, A. T., Crocce, M., da Costa, L. N., Pereira, M. E. S., de Haan, T., De Vicente, J., DeRose, J., Desai, S., Diehl, H. T., Dobbs, M. A., Dodelson, S., Doel, P., Elvin-Poole, J., Everett, W., Everett, S., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gatti, M., George, E. M., Gerdes, D. W., Giannini, G., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Halverson, N. W., Hinton, S. R., Holder, G. P., Hollowood, D. L., Holzapfel, W. L., Honscheid, K., Hrubes, J. D., James, D. J., Knox, L., Kuehn, K., Kuropatkin, N., Lahav, O., Lee, A. T., Luong-Van, D., MacCrann, N., Marshall, J. L., McCullough, J., McMahon, J. J., Melchior, P., Mena-Fernández, J., Menanteau, F., Miquel, R., Mocanu, L., Mohr, J. J., Muir, J., Myles, J., Natoli, T., Padin, S., Palmese, A., Pandey, S., Paz-Chinchón, F., Pieres, A., Malagón, A. A. Plazas, Porredon, A., Pryke, C., Raveri, M., Reichardt, C. L., Rodriguez-Monroy, M., Ross, A. J., Ruhl, J. E., Rykoff, E., Sánchez, C., Sanchez, E., Scarpine, V., Schaffer, K. K., Sevilla-Noarbe, I., Sheldon, E., Shirokoff, E., Smith, M., Soares-Santos, M., Staniszewski, Z., Stark, A. A., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., Troxel, M. A., Tucker, D. L., Vieira, J. D., Vincenzi, M., Weaverdyck, N., Williamson, R., Yanny, B., Yin, B., Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), CEA/DSM Centre de Saclay (CEA/DSM), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), DES, and SPT
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), cosmology: observations, FOS: Physical sciences, galaxies: structure, large-scale structure of Universe, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We cross-correlate positions of galaxies measured in data from the first three years of the Dark Energy Survey with Compton-$y$-maps generated using data from the South Pole Telescope (SPT) and the {\it Planck} mission. We model this cross-correlation measurement together with the galaxy auto-correlation to constrain the distribution of gas in the Universe. We measure the hydrostatic mass bias or, equivalently, the mean halo bias-weighted electron pressure $\langle b_{h}P_{e}\rangle$, using large-scale information. We find $\langle b_{h}P_{e}\rangle$ to be $[0.16^{+0.03}_{-0.04},0.28^{+0.04}_{-0.05},0.45^{+0.06}_{-0.10},0.54^{+0.08}_{-0.07},0.61^{+0.08}_{-0.06},0.63^{+0.07}_{-0.08}]$ meV cm$^{-3}$ at redshifts $z \sim [0.30, 0.46, 0.62,0.77, 0.89, 0.97]$. These values are consistent with previous work where measurements exist in the redshift range. We also constrain the mean gas profile using small-scale information, enabled by the high-resolution of the SPT data. We compare our measurements to different parametrized profiles based on the cosmo-OWLS hydrodynamical simulations. We find that our data are consistent with the simulation that assumes an AGN heating temperature of $10^{8.5}$K but are incompatible with the model that assumes an AGN heating temperature of $10^{8.0}$K. These comparisons indicate that the data prefer a higher value of electron pressure than the simulations within $r_{500c}$ of the galaxies' halos., Comment: 20 pages, 9 figures. Submitted to MNRAS
Published: 2023

7. Cosmological constraints from the tomography of DES-Y3 galaxies with CMB lensing from ACT DR4

Author: Marques, G. A., Madhavacheril, M. S., Darwish, O., Shaikh, S., Aguena, M., Alves, O., Avila, S., Bacon, D., Baxter, E. J., Bechtol, K., Becker, M. R., Bertin, E., Blazek, J., Bond, J. Richard, Brooks, D., Cai, H., Calabrese, E., Rosell, A. Carnero, Carretero, M. Carrasco Kind J., Cawthon, R., Crocce, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Diehl, H. T., Doel, P., Doux, C., Drlica-Wagner, A., Dunkley, J., Elvin-Poole, J., Everett, S., Ferraro, Simone, Ferrero, I., Flaugher, B., Fosalba, P., García-Bellido, J., Gatti, M., Giannini, G., Gluscevic, V., Gruen, D., Gruendl, R. A., Gutierrez, G., Harrison, I., Hill, J. Colin, Hinton, S. R., Hollowood, D. L., Honscheid, K., Huterer, D., Jeffrey, N., Kim, J., Kuehn, K., Lahav, O., Lemos, P., Lima, M., Huffenberger, K. M., MacCrann, N., Marshall, J. L., Mena-Fernández, J., Miquel, R., Mohr, J. J., Moodley, K., Muir, J., Naess, S., Nati, F., Page, L. A., Palmese, A., Malagón, A. A. Plazas, Porredon, A., Prat, J., Qu, F. J., Raveri, M., Ross, A. J., Rykoff, E. S., Farren, G. S., Samuroff, S., Sanchez, E., Schubnell, M., Sevilla-Noarbe, I., Sheldon, E., Sherwin, B. D., Sifón, C., Smith, M., Spergel, D. N., Staggs, S. T., Suchyta, E., Tarle, G., To, C., Van Engelen, A., Weaverdyck, N., Weller, J., Wenzl, L., Wiseman, P., Wollack, E. J., and Yanny, B.
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present a measurement of the cross-correlation between the MagLim galaxies selected from the Dark Energy Survey (DES) first three years of observations (Y3) and cosmic microwave background (CMB) lensing from the Atacama Cosmology Telescope (ACT) Data Release 4 (DR4), reconstructed over $\sim 436$ sq.deg. of the sky. Our galaxy sample, which covers $\sim 4143$ sq.deg., is divided into six redshift bins spanning the redshift range of $0.20, Comment: 42 pages, 17 figures
Published: 2023
Full Text: View/download PDF

8. Dark Energy Survey Year 3 results: Constraints on extensions to Λ CDM with weak lensing and galaxy clustering

Author: Abbott, T. M. C., Aguena, M., Alarcon, A., Alves, O., Amon, A., Andrade-Oliveira, F., Annis, J., Avila, S., Bacon, D., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Birrer, S., Blazek, J., Bocquet, S., Brandao-Souza, A., Bridle, S. L., Brooks, D., Burke, D. L., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Cawthon, R., Chang, C., Chen, A., Chen, R., Choi, A., Conselice, C., Cordero, J., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., Davis, C., Davis, T. M., Derose, J., Desai, S., Di Valentino, E., Diehl, H. T., Dodelson, S., Doel, P., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Elvin-Poole, J., Everett, S., Fang, X., Farahi, A., Ferrero, I., Ferté, A., Flaugher, B., Fosalba, P., Friedel, D., Friedrich, O., Frieman, J., García-Bellido, J., Gatti, M., Giani, L., Giannantonio, T., Giannini, G., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hamaus, N., Harrison, I., Hartley, W. G., Herner, K., Hinton, S. R., Hollowood, D. L., Honscheid, K., Huang, H., Huff, E. M., Huterer, D., Jain, B., James, D. J., Jarvis, M., Jeffrey, N., Jeltema, T., Kovacs, A., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lee, S., Leget, P. -F., Lemos, P., Leonard, C. D., Liddle, A. R., Lima, M., Lin, H., Maccrann, N., Marshall, J. L., Mccullough, J., Mena-Fernández, J., Menanteau, F., Miquel, R., Miranda, V., Mohr, J. J., Muir, J., Myles, J., Nadathur, S., Navarro-Alsina, A., Nichol, R. C., Ogando, R. L. C., Omori, Y., Palmese, A., Pandey, S., Park, Y., Paterno, M., Paz-Chinchón, F., Percival, W. J., Pieres, A., Plazas Malagón, A. A., Porredon, A., Prat, J., Raveri, M., Rodriguez-Monroy, M., Rogozenski, P., Rollins, R. P., Romer, A. K., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, E., Sanchez, J., Sanchez Cid, D., Scarpine, V., Scolnic, D., Secco, L. F., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Smith, M., Soares-Santos, M., Suchyta, E., Tabbutt, M., Tarle, G., Thomas, D., To, C., Troja, A., Troxel, M. A., Tutusaus, I., Varga, T. N., Vincenzi, M., Walker, A. R., Weaverdyck, N., Wechsler, R. H., Weller, J., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., and Des, Collaboration
Published: 2023

9. Tapping fashion market niches for organic agroforestry cotton: new marketsʼ potential for promoting sustainable supply chains

Author: Mwabonje, O, Coelho e Silva, R, De Siqueira Camargo, R, Da Silva Medina, G, Gatti, M, and Sevigne Itoiz, E
Abstract: We hypothesize that Fashion brands’ demand for organic agroforestry cotton (OAC) may foster more sustainable supply chains in the cotton industry. However, to realize the potential of the OAC market, a better understanding of the market demand for OAC, as well as the quality and production standards under which the brands operate, the institutional frameworks, and the market mechanisms that underpin its commercialization, is needed. We evaluated the existing organic markets in Brazil using an interview-based methodology with key stakeholders throughout the organic cotton supply chain in 2022. Our study revealed that some brands are willing to pay prices ranging from USD$ 2.57 to USD$ 4.61 per kg of cotton lint depending on the brand. These brands require suppliers to meet quality specifications for the cotton fiber; for example, they require average to long fibers and specify harvesting practices that influence fiber quality. There are also social and environmental criteria that prioritize vulnerable communities of family farmers and women groups planting cotton based on established sustainable practices. The institutional framework includes different stakeholders throughout the organic cotton supply chain, which is fundamentally driven by private demand for cotton, counts on the support of agents connecting brands to farmers, and is indirectly supported by public policies. Existing markets for organic cotton are established via contracts that provide farmers with guarantees to invest in planting cotton and have different certification systems used by the brands that monitor and verify adherence to the standards. Market demand for OAC may, therefore, potentially lead to new markets that promote sustainable supply chains and farming practices. However, existing markets for organic cotton reveal complex requirements that must be addressed, such as the need for supporting agents connecting brands to farmers, and market mechanisms, such as complex contracts and certification.
Published: 2022

10. The Dark Energy Survey Year 3 and eBOSS: constraining galaxy intrinsic alignments across luminosity and colour space

Author: Samuroff, S., Mandelbaum, R., Blazek, J., Campos, A., MacCrann, N., Zacharegkas, G., Amon, A., Prat, J., Singh, S., Elvin-Poole, J., Ross, A. J., Alarcon, A., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Rosell, A. Carnero, Kind, M. Carrasco, Cawthon, R., Chang, C., Chen, R., Choi, A., Crocce, M., Davis, C., DeRose, J., Dodelson, S., Doux, C., Drlica-Wagner, A., Eckert, K., Everett, S., Ferté, A., Gatti, M., Giannini, G., Gruen, D., Gruendl, R. A., Harrison, I., Herner, K., Huff, E. M., Jarvis, M., Kuropatkin, N., Leget, P. -F., Lemos, P., McCullough, J., Myles, J., Navarro-Alsina, A., Pandey, S., Porredon, A., Raveri, M., Rodriguez-Monroy, M., Rollins, R. P., Roodman, A., Rossi, G., Rykoff, E. S., Sánchez, C., Secco, L. F., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troxel, M. A., Tutusaus, I., Weaverdyck, N., Yanny, B., Yin, B., Zhang, Y., Aguena, J. Zuntz M., Alves, O., Annis, J., Bacon, D., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., Marshall, J. L., Melchior, P., Mena-Fernández, J., Menanteau, F., Miquel, R., Newman, J., Palmese, A., Pieres, A., Malagón, A. A. Plazas, Sanchez, E., Scarpine, V., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., and To, C.
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present direct constraints on galaxy intrinsic alignments using the Dark Energy Survey Year 3 (DES Y3), the Extended Baryon Oscillation Spectroscopic Survey (eBOSS) and its precursor, the Baryon Oscillation Spectroscopic Survey (BOSS). Our measurements incorporate photometric red sequence (redMaGiC) galaxies from DES with median redshift $z\sim0.2-1.0$, luminous red galaxies (LRGs) from eBOSS at $z\sim0.8$, and also a SDSS-III BOSS CMASS sample at $z\sim0.5$. We measure two point intrinsic alignment correlations, which we fit using a model that includes lensing, magnification and photometric redshift error. Fitting on scales $6, Comment: Submitted to MNRAS; 22 pages, 11 figures
Published: 2022

11. A Sample of Dust Attenuation Laws for DES Supernova Host Galaxies

Author: Duarte, J., González-Gaitán, S., Mourao, A., Paulino-Afonso, A., Guilherme-Garcia, P., Aguas, J., Galbany, L., Kelsey, L., Scolnic, D., Sullivan, M., Brout, D., Palmese, A., Wiseman, P., Pieres, A., Malagón, A. A. Plazas, Rosell, A. Carnero, To, C., Gruen, D., Bacon, D., Brooks, D., Burke, D. L., Gerdes, D. W., James, D. J., Hollowood, D. L., Friedel, D., Bertin, E., Suchyta, E., Sanchez, E., Paz-Chinchón, F., Gutierrez, G., Tarle, G., Diehl, H. T., Sevilla-Noarbe, I., Ferrero, I., Carretero, J., Frieman, J., De Vicente, J., García-Bellido, J., Honscheid, K., Kuehn, K., Gatti, M., Raveri, M., Pereira, M. E. S., Rodriguez-Monroy, M., Smith, M., Kind, M. Carrasco, Costanzi, M., Aguena, M., Kuropatkin, N., Weaverdyck, N., Alves, O., Doel, P., Melchior, P., Miquel, R., Gruendl, R. A., Hinton, S. R., Bocquet, S., Desai, S., Everett, S., Davis, T. M., Scarpine, V., and HEP, INSPIRE
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Astrophysics of Galaxies (astro-ph.GA), FOS: Physical sciences, [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Type Ia supernovae (SNe Ia) are useful distance indicators in cosmology, provided their luminosity is standardized by applying empirical corrections based on light-curve properties. One factor behind these corrections is dust extinction, accounted for in the color-luminosity relation of the standardization. This relation is usually assumed to be universal, which could potentially introduce systematics into the standardization. The ``mass-step'' observed for SNe Ia Hubble residuals has been suggested as one such systematic. We seek to obtain a completer view of dust attenuation properties for a sample of 162 SN Ia host galaxies and to probe their link to the ``mass-step''. We infer attenuation laws towards hosts from both global and local (4 kpc) Dark Energy Survey photometry and Composite Stellar Population model fits. We recover a optical depth/attenuation slope relation, best explained by differing star/dust geometry for different galaxy orientations, which is significantly different from the optical depth/extinction slope relation observed directly for SNe. We obtain a large variation of attenuation slopes and confirm these change with host properties, like stellar mass and age, meaning a universal SN Ia correction should ideally not be assumed. Analyzing the cosmological standardization, we find evidence for a ``mass-step'' and a two dimensional ``dust-step'', both more pronounced for red SNe. Although comparable, the two steps are found no to be completely analogous. We conclude that host galaxy dust data cannot fully account for the ``mass-step'', using either an alternative SN standardization with extinction proxied by host attenuation or a ``dust-step'' approach., 20 pages, 10 figues, 9 tables. Supplementary material included (10 pages). Submitted to MNRAS
Published: 2022

12. A galaxy-driven model of type Ia supernova luminosity variations

Author: Wiseman, P., Vincenzi, M., Sullivan, M., Kelsey, L., Popovic, B., Rose, B., Brout, D., Davis, T. M., Frohmaier, C., Galbany, L., Lidman, C., Möller, A., Scolnic, D., Smith, M., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Costanzi, M., Pereira, M. E. S., Desai, S., Diehl, H. T., Doel, P., Everett, S., Ferrero, I., Friedel, D., Frieman, J., García-Bellido, J., Gatti, M., Gaztanaga, E., Gruen, D., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., March, M., Menanteau, F., Miquel, R., Morgan, R., Palmese, A., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A. A., Romer, A. K., Sanchez, E., Scarpine, V., Sevilla-Noarbe, I., Soares-Santos, M., Suchyta, E., Tarle, G., To, C., Varga, T. N., DES Collaboration, Wiseman, P., Vincenzi, M., Sullivan, M., Kelsey, L., Popovic, B., Rose, B., Brout, D., Davis, T. M., Frohmaier, C., Galbany, L., Lidman, C., Möller, A., Scolnic, D., Smith, M., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Costanzi, M., Pereira, M. E. S., Desai, S., Diehl, H. T., Doel, P., Everett, S., Ferrero, I., Friedel, D., Frieman, J., García-Bellido, J., Gatti, M., Gaztanaga, E., Gruen, D., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., March, M., Menanteau, F., Miquel, R., Morgan, R., Palmese, A., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A. A., Romer, A. K., Sanchez, E., Scarpine, V., Sevilla-Noarbe, I., Soares-Santos, M., Suchyta, E., Tarle, G., To, C., Varga, T. N., Des, Collaboration, Science and Technology Facilities Council (UK), European Commission, Ministerio de Ciencia, Innovación y Universidades (España), Agencia Estatal de Investigación (España), Consejo Superior de Investigaciones Científicas (España), European Research Council, Department of Energy (US), National Science Foundation (US), Ministerio de Educación y Ciencia (España), and Generalitat de Catalunya
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), supernovae general, dust, extinction, galaxies evolution, cosmology observations, Cosmology: observations, Supernovae: general, Galaxies: evolution, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - Astrophysics of Galaxies, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: DES Collaboration: P. Wiseman et al., Type Ia supernovae (SNe Ia) are used as standardizable candles to measure cosmological distances, but differences remain in their corrected luminosities which display a magnitude step as a function of host galaxy properties such as stellar mass and rest-frame U−R colour. Identifying the cause of these steps is key to cosmological analyses and provides insight into SN physics. Here we investigate the effects of SN progenitor ages on their light-curve properties using a galaxy-based forward model that we compare to the Dark Energy Survey 5-yr SN Ia sample. We trace SN Ia progenitors through time and draw their light-curve width parameters from a bimodal distribution according to their age. We find that an intrinsic luminosity difference between SNe of different ages cannot explain the observed trend between step size and SN colour. The data split by stellar mass are better reproduced by following recent work implementing a step in total-to-selective dust extinction ratio (RV) between low- and high-mass hosts, although an additional intrinsic luminosity step is still required to explain the data split by host galaxy U−R. Modelling the RV step as a function of galaxy age provides a better match overall. Additional age versus luminosity steps marginally improve the match to the data, although most of the step is absorbed by the width versus luminosity coefficient α. Furthermore, we find no evidence that α varies with SN age., P.W. acknowledges support from the Science and Technology Facilities Council (STFC) grant ST/R000506/1. MS acknowledges support from EU/FP7-ERC grant 615929. LK thanks the UKRI Future Leaders Fellowship for support through the grant MR/T01881X/1. LG acknowledges financial support from the Spanish Ministerio de Ciencia e Innovación (MCIN), the Agencia Estatal de Investigación (AEI) 10.13039/501100011033, and the European Social Fund (ESF) ‘Investing in your future’ under the 2019 Ramón y Cajal program RYC2019-027683-I and the PID2020-115253GA-I00 HOSTFLOWS project, from Centro Superior de Investigaciones Científicas (CSIC) under the PIE project 20215AT016, and the program Unidad de Excelencia María de Maeztu CEX2020-001058-M. This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement number 759194 - USNAC). Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft, and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciències de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, NSF’s NOIRLab, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. Based in part on observations at Cerro Tololo Inter-American Observatory at NSF’s NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under Grant Numbers AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under grants ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq grant 465376/2014-2). This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics.
Published: 2022

13. Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to modeling uncertainty

Author: Secco, L. F., Samuroff, S., Krause, E., Jain, B., Blazek, J., Raveri, M., Campos, A., Amon, A., Chen, A., Doux, C., Choi, A., Gruen, D., Bernstein, G. M., Chang, C., Derose, J., Myles, J., Ferté, A., Lemos, P., Huterer, D., Prat, J., Troxel, M. A., Maccrann, N., Liddle, A. R., Kacprzak, T., Fang, X., Sánchez, C., Pandey, S., Dodelson, S., Chintalapati, P., Hoffmann, K., Alarcon, A., Alves, O., Andrade-Oliveira, F., Baxter, E. J., Bechtol, K., Becker, M. R., Brandao-Souza, A., Camacho, H., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Cordero, J. P., Crocce, M., Davis, C., Di Valentino, E., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elidaiana, M., Elsner, F., Elvin-Poole, J., Everett, S., Fosalba, P., Friedrich, O., Gatti, M., Giannini, G., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Huang, H., Huff, E. M., Jarvis, M., Jeffrey, N., Kuropatkin, N., Leget, P. -F., Muir, J., Mccullough, J., Navarro Alsina, A., Omori, Y., Park, Y., Porredon, A., Rollins, R., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Sanchez, J., Sevilla-Noarbe, I., Sheldon, E. S., Shin, T., Troja, A., Tutusaus, I., Varga, T. N., Weaverdyck, N., Wechsler, R. H., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Bhargava, S., Bridle, S. L., Brooks, D., Buckley-Geer, E., Burke, D. L., Carretero, J., Costanzi, M., da Costa, L. N., De Vicente, J., Diehl, H. T., Dietrich, J. P., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Jeltema, T., Kuehn, K., Lahav, O., Lima, M., Lin, H., Maia, M. A. G., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Petravick, D., Pieres, A., Plazas Malagón, A. A., Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Scarpine, V., Schubnell, M., Scolnic, D., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Des, Collaboration, Laboratoire de physique de l'ENS - ENS Paris (LPENS), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)-Département de Physique de l'ENS-PSL, École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École normale supérieure - Paris (ENS-PSL), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), DES, Secco, L. F., Samuroff, S., Krause, E., Jain, B., Blazek, J., Raveri, M., Campos, A., Amon, A., Chen, A., Doux, C., Choi, A., Gruen, D., Bernstein, G. M., Chang, C., Derose, J., Myles, J., Ferte, A., Lemos, P., Huterer, D., Prat, J., Troxel, M. A., Maccrann, N., Liddle, A. R., Kacprzak, T., Fang, X., Sanchez, C., Pandey, S., Dodelson, S., Chintalapati, P., Hoffmann, K., Alarcon, A., Alves, O., Andrade-Oliveira, F., Baxter, E. J., Bechtol, K., Becker, M. R., Brandao-Souza, A., Camacho, H., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Cordero, J. P., Crocce, M., Davis, C., Di Valentino, E., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elidaiana, M., Elsner, F., Elvin-Poole, J., Everett, S., Fosalba, P., Friedrich, O., Gatti, M., Giannini, G., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Huang, H., Huff, E. M., Jarvis, M., Jeffrey, N., Kuropatkin, N., Leget, P. -F., Muir, J., Mccullough, J., Navarro Alsina, A., Omori, Y., Park, Y., Porredon, A., Rollins, R., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Sanchez, J., Sevilla-Noarbe, I., Sheldon, E. S., Shin, T., Tutusaus, I., Varga, T. N., Weaverdyck, N., Wechsler, R. H., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Bhargava, S., Bridle, S. L., Brooks, D., Buckley-Geer, E., Burke, D. L., Carretero, J., Costanzi, M., Da Costa, L. N., De Vicente, J., Diehl, H. T., Dietrich, J. P., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., Garcia-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Jeltema, T., Kuehn, K., Lahav, O., Lima, M., Lin, H., Maia, M. A. G., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Palmese, A., Paz-Chinchon, F., Petravick, D., Pieres, A., Plazas Malagon, A. A., Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Scarpine, V., Schubnell, M., Scolnic, D., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Sorbonne Université (SU)-École normale supérieure - Paris (ENS Paris), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), National Science Foundation (US), European Commission, Ministerio de Economía y Competitividad (España), Generalitat de Catalunya, Australian Research Council, University of Chicago, University of Pennsylvania, Carnegie Mellon University, Northeastern University, University of Arizona, École Polytechnique Fédérale de Lausanne (EPFL), Stanford University, University of Michigan, The Ohio State University, 382 Via Pueblo Mall, SLAC National Accelerator Laboratory, University of California, California Institute of Technology, University College London, Duke University, University of Cambridge, Universidade de Lisboa, University of Edinburgh, Perimeter Institute for Theoretical Physics, ETH Zürich, Northern Illinois University, University of Zürich, Argonne National Laboratory, Universidade Estadual Paulista (UNESP), Laboratório Interinstitucional de E-Astronomia - LIneA, University of Hawai'i, University of Wisconsin-Madison, Universidade Estadual de Campinas (UNICAMP), Medioambientales y Tecnológicas (CIEMAT), Instituto de Astrofísica de Canarias, Dpto. Astrofísica, University of Illinois at Urbana-Champaign, National Center for Supercomputing Applications, University of Manchester, Institut d'Estudis Espacials de Catalunya (IEEC), Institute of Space Sciences (ICE CSIC), Fermi National Accelerator Laboratory, Max Planck Institute für Extraterrestrial Physics, Santa Cruz Institute for Particle Physics, The Barcelona Institute of Science and Technology, Denys Wilkinson Building, Université de Genève, Université de Paris, Laboratoire de Physique de Clermont, Laboratoire de Physique Nucléaire et de Hautes Énergies, The University of Tokyo, Ohio State University, Brookhaven National Laboratory, Ludwig-Maximilians Universität München, NSF's National Optical-Infrared Astronomy Research Laboratory, University of Portsmouth, Institut d'Astrophysique de Paris, University of Sussex, University of Trieste, INAF-Osservatorio Astronomico di Trieste, Institute for Fundamental Physics of the Universe, Observatório Nacional, Ludwig-Maximilians-Universität, University of Oslo, Universidad Autonoma de Madrid, University of Queensland, Max Planck Institute for Extraterrestrial Physics, Center for Astrophysics | Harvard and Smithsonian, Macquarie University, Lowell Observatory, Universidade de São Paulo (USP), Texas A and M University, Harvard University, Peyton Hall, Institució Catalana de Recerca i Estudis Avançats, University of Southampton, Oak Ridge National Laboratory, Laboratoire de physique de l'ENS - ENS Paris (LPENS (UMR_8023)), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), and UAM. Departamento de Física Teórica
Subjects: luminous red galaxies, Cosmology and Nongalactic Astrophysics (astro-ph.CO), challenge lightcone simulation, Cosmological parameters, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, power spectrum, Sky surveys, Astrophysics, 01 natural sciences, large-scale structure, Astrophysic, weak-lensing surveys, Gravitational lenses, Cosmology and Nongalactic Astrophysics, 0103 physical sciences, Weak, baryonic feedback, 010303 astronomy & astrophysics, redshift inference, intrinsic galaxy shapes, Gravitational Lensing, 010308 nuclear & particles physics, Física, COSMOLOGIA, Dark Energy, 13. Climate action, 2-point correlation-functions, photometric data set, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Secco, L.F., et al. (DES Collaboration), This work and its companion paper, Amon et al. [Phys. Rev. D 105, 023514 (2022)PRVDAQ2470-001010.1103/PhysRevD.105.023514], present cosmic shear measurements and cosmological constraints from over 100 million source galaxies in the Dark Energy Survey (DES) Year 3 data. We constrain the lensing amplitude parameter S8σ8ωm/0.3 at the 3% level in ΛCDM: S8=0.759-0.023+0.025 (68% CL). Our constraint is at the 2% level when using angular scale cuts that are optimized for the ΛCDM analysis: S8=0.772-0.017+0.018 (68% CL). With cosmic shear alone, we find no statistically significant constraint on the dark energy equation-of-state parameter at our present statistical power. We carry out our analysis blind, and compare our measurement with constraints from two other contemporary weak lensing experiments: the Kilo-Degree Survey (KiDS) and Hyper-Suprime Camera Subaru Strategic Program (HSC). We additionally quantify the agreement between our data and external constraints from the Cosmic Microwave Background (CMB). Our DES Y3 result under the assumption of ΛCDM is found to be in statistical agreement with Planck 2018, although favors a lower S8 than the CMB-inferred value by 2.3σ (a p-value of 0.02). This paper explores the robustness of these cosmic shear results to modeling of intrinsic alignments, the matter power spectrum and baryonic physics. We additionally explore the statistical preference of our data for intrinsic alignment models of different complexity. The fiducial cosmic shear model is tested using synthetic data, and we report no biases greater than 0.3σ in the plane of S8×ωm caused by uncertainties in the theoretical models., The DES data management system is supported by the National Science Foundation under Grants No. AST-1138766 and No. AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under Grants No. AYA2015-71825, No. ESP2015-88861, No. FPA2015-68048, No. SEV-2012-0234, No. SEV-2016-0597, and No. MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC grant agreements No. 240672, No. 291329, and No. 306478. We acknowledge support from the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020.
Published: 2022

14. Milky Way Satellite Census. IV. Constraints on Decaying Dark Matter from Observations of Milky Way Satellite Galaxies

Author: A Mau, S., Nadler, E. O., Wechsler, R. H., Drlica-Wagner, A., Bechtol, K., Green, G., Huterer, D., Li, T. S., Mao, Y. -Y., Martínez-Vázquez, C. E., McNanna, M., Mutlu-Pakdil, B., Pace, A. B., Peter, A., Riley, A. H., Strigari, L., Wang, M. -Y., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Costanzi, M., Crocce, M., Pereira, M. E. S., Davis, T. M., Vicente, J. De, Desai, S., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gatti, M., Giannini, G., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., Maia, M. A. G., Marshall, J. L., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Paz-Chinchón, F., Pieres, A., Rodriguez-Monroy, M., Sanchez, E., Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Suchyta, E., Tarle, G., To, C., Tucker, D. L., Weller, J., DES Collaboration, Mau, S [0000-0003-3519-4004], Nadler, EO [0000-0002-1182-3825], Wechsler, RH [0000-0003-2229-011X], Drlica-Wagner, A [0000-0001-8251-933X], Bechtol, K [0000-0001-8156-0429], Green, G [0000-0001-5417-2260], Huterer, D [0000-0001-6558-0112], Li, TS [0000-0002-9110-6163], Mao, YY [0000-0002-1200-0820], Martínez-Vázquez, CE [0000-0002-9144-7726], McNanna, M [0000-0001-5435-7820], Mutlu-Pakdil, B [0000-0001-9649-4815], Pace, AB [0000-0002-6021-8760], Peter, A [0000-0002-8040-6785], Riley, AH [0000-0001-5805-5766], Strigari, L [0000-0001-5672-6079], Wang, MY [0000-0002-8226-6237], Aguena, M [0000-0001-5679-6747], Allam, S [0000-0002-7069-7857], Annis, J [0000-0002-0609-3987], Bacon, D [0000-0002-2562-8537], Bertin, E [0000-0002-3602-3664], Bocquet, S [0000-0002-4900-805X], Brooks, D [0000-0002-8458-5047], Burke, DL [0000-0003-1866-1950], Rosell, AC [0000-0003-3044-5150], Kind, MC [0000-0002-4802-3194], Carretero, J [0000-0002-3130-0204], Costanzi, M [0000-0001-8158-1449], Crocce, M [0000-0002-9745-6228], Davis, TM [0000-0002-4213-8783], Vicente, JD [0000-0001-8318-6813], Desai, S [0000-0002-0466-3288], Ferrero, I [0000-0002-1295-1132], Flaugher, B [0000-0002-2367-5049], Frieman, J [0000-0003-4079-3263], García-Bellido, J [0000-0002-9370-8360], Giannini, G [0000-0002-3730-1750], Gruen, D [0000-0003-3270-7644], Gruendl, RA [0000-0002-4588-6517], Gschwend, J [0000-0003-3023-8362], Gutierrez, G [0000-0003-0825-0517], Hinton, SR [0000-0003-2071-9349], Hollowood, DL [0000-0002-9369-4157], Honscheid, K [0000-0002-6550-2023], James, DJ [0000-0001-5160-4486], Kuehn, K [0000-0003-0120-0808], Lahav, O [0000-0002-1134-9035], Maia, MAG [0000-0001-9856-9307], Marshall, JL [0000-0003-0710-9474], Miquel, R [0000-0002-6610-4836], Morgan, R [0000-0002-7016-5471], Ogando, RLC [0000-0003-2120-1154], Paz-Chinchón, F [0000-0003-1339-2683], Pieres, A [0000-0001-9186-6042], Sanchez, E [0000-0002-9646-8198], Serrano, S [0000-0002-0211-2861], Sevilla-Noarbe, I [0000-0002-1831-1953], Suchyta, E [0000-0002-7047-9358], Tarle, G [0000-0003-1704-0781], To, C [0000-0001-7836-2261], Tucker, DL [0000-0001-7211-5729], Weller, J [0000-0002-8282-2010], Apollo - University of Cambridge Repository, UAM. Departamento de Física Teórica, Department of Energy (US), National Science Foundation (US), Ministerio de Educación y Ciencia (España), Kavli Institute for Particle Astrophysics and Cosmology, Science and Technology Facilities Council (UK), Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico (Brasil), Ministerio de Economía y Competitividad (España), German Research Foundation, Agencia Estatal de Investigación (España), Ministerio de Ciencia, Innovación y Universidades (España), European Commission, Generalitat de Catalunya, European Research Council, A Mau, S., Nadler, E. O., Wechsler, R. H., Drlica-Wagner, A., Bechtol, K., Green, G., Huterer, D., T. S., Li, Mao, Y. -Y., Martínez-Vázquez, C. E., Mcnanna, M., Mutlu-Pakdil, B., Pace, A. B., Peter, A., Riley, A. H., Strigari, L., Wang, M. -Y., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Costanzi, M., Crocce, M., Pereira, M. E. S., Davis, T. M., Vicente, J. De, Desai, S., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gatti, M., Giannini, G., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., Maia, M. A. G., Marshall, J. L., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Paz-Chinchón, F., Pieres, A., Rodriguez-Monroy, M., Sanchez, E., Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Suchyta, E., Tarle, G., To, C., Tucker, D. L., Weller, J., and Des, Collaboration
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), astro-ph.GA, FOS: Physical sciences, Física, Astronomy and Astrophysics, hep-ph, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - Astrophysics of Galaxies, Galaxy abundances, High Energy Physics - Phenomenology, Halo, High Energy Physics - Phenomenology (hep-ph), Dwarf Galaxies, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Dark matter, astro-ph.CO, Dark Matter, Milky Way dark matter halo, Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Mau et al., We use a recent census of the Milky Way (MW) satellite galaxy population to constrain the lifetime of particle dark matter (DM). We consider two-body decaying dark matter (DDM) in which a heavy DM particle decays with lifetime τ comparable to the age of the universe to a lighter DM particle (with mass splitting epsilon) and to a dark radiation species. These decays impart a characteristic "kick velocity," Vkick = epsilonc, on the DM daughter particles, significantly depleting the DM content of low-mass subhalos and making them more susceptible to tidal disruption. We fit the suppression of the present-day DDM subhalo mass function (SHMF) as a function of τ and Vkick using a suite of high-resolution zoom-in simulations of MW-mass halos, and we validate this model on new DDM simulations of systems specifically chosen to resemble the MW. We implement our DDM SHMF predictions in a forward model that incorporates inhomogeneities in the spatial distribution and detectability of MW satellites and uncertainties in the mapping between galaxies and DM halos, the properties of the MW system, and the disruption of subhalos by the MW disk using an empirical model for the galaxy–halo connection. By comparing to the observed MW satellite population, we conservatively exclude DDM models with τ < 18 Gyr (29 Gyr) for Vkick = 20 kms−1 (40 kms−1) at 95% confidence. These constraints are among the most stringent and robust small-scale structure limits on the DM particle lifetime and strongly disfavor DDM models that have been proposed to alleviate the Hubble and S8 tensions., Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft, and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciències de l'Espai (IEEC/CSIC), the Institut de Física d'Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, NSF's NOIRLab, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. Based in part on observations at Cerro Tololo Inter-American Observatory at NSF's NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under grant No. AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under grants ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Program (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq grant 465376/2014-2). This manuscript has been authored by Fermi Research Alliance, LLC under contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics.
Published: 2022

15. Measuring Cosmological Parameters with Type Ia Supernovae in redMaGiC Galaxies

Author: Chen, R, Scolnic, D, Rozo, E, Rykoff, ES, Popovic, B, Kessler, R, Vincenzi, M, Davis, TM, Armstrong, P, Brout, D, Galbany, L, Kelsey, L, Lidman, C, Möller, A, Rose, B, Sako, M, Sullivan, M, Taylor, G, Wiseman, P, Asorey, J, Carr, A, Conselice, C, Kuehn, K, Lewis, GF, Macaulay, E, Rodriguez-Monroy, M, Tucker, BE, Abbott, TMC, Aguena, M, Allam, S, Andrade-Oliveira, F, Annis, J, Bacon, D, Bertin, E, Bocquet, S, Brooks, D, Burke, DL, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Cawthon, R, Costanzi, M, Da Costa, LN, Pereira, MES, Desai, S, Diehl, HT, Doel, P, Everett, S, Ferrero, I, Flaugher, B, Friedel, D, Frieman, J, García-Bellido, J, Gatti, M, Gaztanaga, E, Gruen, D, Hinton, Hollowood, DL, Honscheid, K, James, DJ, Lahav, O, Lima, M, March, M, Menanteau, F, Miquel, R, Morgan, R, Palmese, A, Paz-Chinchón, F, Pieres, A, Plazas Malagón, AA, Prat, J, Romer, AK, Roodman, A, Sanchez, E, Schubnell, M, Serrano, S, Sevilla-Noarbe, I, Smith, M, Soares-Santos, M, Suchyta, E, Tarle, G, Thomas, D, To, C, Tucker, DL, Varga, TN, Department of Energy (US), National Aeronautics and Space Administration (US), National Science Foundation (US), Agencia Estatal de Investigación (España), Ministerio de Ciencia, Innovación y Universidades (España), Generalitat de Catalunya, European Commission, European Research Council, Chen, R., Scolnic, D., Rozo, E., Rykoff, E. S., Popovic, B., Kessler, R., Vincenzi, M., Davis, T. M., Armstrong, P., Brout, D., Galbany, L., Kelsey, L., Lidman, C., Möller, A., Rose, B., Sako, M., Sullivan, M., Taylor, G., Wiseman, P., Asorey, J., Carr, A., Conselice, C., Kuehn, K., Lewis, G. F., Macaulay, E., Rodriguez-Monroy, M., Tucker, B. E., Abbott, T. M. C., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bacon, D., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Cawthon, R., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Desai, S., Diehl, H. T., Doel, P., Everett, S., Ferrero, I., Flaugher, B., Friedel, D., Frieman, J., García-Bellido, J., Gatti, M., Gaztanaga, E., Gruen, D., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Lahav, O., Lima, M., March, M., Menanteau, F., Miquel, R., Morgan, R., Palmese, A., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A. A., Prat, J., Romer, A. K., Roodman, A., Sanchez, E., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Tucker, D. L., Varga, T. N., Chen, R [0000-0003-3917-0966], Rykoff, ES [0000-0001-9376-3135], Popovic, B [0000-0002-8012-6978], Kessler, R [0000-0003-3221-0419], Davis, TM [0000-0002-4213-8783], Brout, D [0000-0001-5201-8374], Galbany, L [0000-0002-1296-6887], Lidman, C [0000-0003-1731-0497], Sako, M [0000-0003-2764-7093], Sullivan, M [0000-0001-9053-4820], Carr, A [0000-0003-4074-5659], Conselice, C [0000-0003-1949-7638], Kuehn, K [0000-0003-0120-0808], Lewis, GF [0000-0003-3081-9319], Tucker, BE [0000-0002-4283-5159], Aguena, M [0000-0001-5679-6747], Annis, J [0000-0002-0609-3987], Bacon, D [0000-0002-2562-8537], Bertin, E [0000-0002-3602-3664], Bocquet, S [0000-0002-4900-805X], Brooks, D [0000-0002-8458-5047], Carretero, J [0000-0002-3130-0204], Costanzi, M [0000-0001-8158-1449], Desai, S [0000-0002-0466-3288], Diehl, HT [0000-0002-8357-7467], García-Bellido, J [0000-0002-9370-8360], Gaztanaga, E [0000-0001-9632-0815], Gruen, D [0000-0003-3270-7644], Hinton, SR [0000-0003-2071-9349], Hollowood, DL [0000-0002-9369-4157], Menanteau, F [0000-0002-1372-2534], Miquel, R [0000-0002-6610-4836], Morgan, R [0000-0002-7016-5471], Palmese, A [0000-0002-6011-0530], Paz-Chinchón, F [0000-0003-1339-2683], Pieres, A [0000-0001-9186-6042], Romer, AK [0000-0002-9328-879X], Roodman, A [0000-0001-5326-3486], Serrano, S [0000-0002-0211-2861], Sevilla-Noarbe, I [0000-0002-1831-1953], Smith, M [0000-0002-3321-1432], Soares-Santos, M [0000-0001-6082-8529], Tarle, G [0000-0003-1704-0781], Thomas, D [0000-0002-6325-5671], Tucker, DL [0000-0001-7211-5729], and Apollo - University of Cambridge Repository
Subjects: Type Ia supernovae, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cosmology, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, COSMOLOGIA, 5109 Space Sciences, Space and Planetary Science, Astrophysics::Solar and Stellar Astrophysics, Astrophysics::Earth and Planetary Astrophysics, 51 Physical Sciences, Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: DES Collaboration: Chen et al., Current and future cosmological analyses with Type Ia supernovae (SNe Ia) face three critical challenges: (i) measuring the redshifts from the SNe or their host galaxies; (ii) classifying the SNe without spectra; and (iii) accounting for correlations between the properties of SNe Ia and their host galaxies. We present here a novel approach that addresses each of these challenges. In the context of the Dark Energy Survey (DES), we analyze an SN Ia sample with host galaxies in the redMaGiC galaxy catalog, a selection of luminous red galaxies. redMaGiC photo-z estimates are expected to be accurate to σΔz/(1+z) ∼ 0.02. The DES-5YR photometrically classified SN Ia sample contains approximately 1600 SNe, and 125 of these SNe are in redMaGiC galaxies. We demonstrate that redMaGiC galaxies almost exclusively host SNe Ia, reducing concerns relating to classification uncertainties. With this subsample, we find similar Hubble scatter (to within ∼0.01 mag) using photometric redshifts in place of spectroscopic redshifts. With detailed simulations, we show that the bias due to using redMaGiC photo-zs on the measurement of the dark energy equation of state w is up to Δw ∼ 0.01–0.02. With real data, we measure a difference in w when using the redMaGiC photo-zs versus the spec-zs of Δw = 0.005. Finally, we discuss how SNe in redMaGiC galaxies appear to comprise a more standardizable population, due to a weaker relation between color and luminosity (β) compared to the DES-3YR population by ∼5σ. These results establish the feasibility of performing redMaGiC SN cosmology with photometric survey data in the absence of spectroscopic data., D.S. is supported by DOE grant No. DE-SC0010007 and the David and Lucile Packard Foundation. D.S. is supported in part by NASA under Contract No. NNG17PX03C, issued through the WFIRST Science Investigation Teams Programme. E. Rozo is supported by NSF grant No. 2009401. E. Rozo is further supported by DOE grant No. DE-SC0009913 and by a Cottrell Scholar award. L.K. thanks the UKRI Future Leaders Fellowship for support through grant No. MR/T01881X/1. L.G. acknowledges financial support from the Spanish Ministry of Science and Innovation (MCIN) under the 2019 Ramón y Cajal program RYC2019-027683-I and from the Spanish MCIN project HOSTFLOWS PID2020-115253GA-I00. This paper has gone through internal review by the DES collaboration. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft, and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciències de l'Espai (IEEC/CSIC), the Institut de Física d'Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, NFS's NOIRLab, the University of Nottingham, the Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. Based in part on observations at Cerro Tololo Inter-American Observatory at NSF's NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under grant Nos. AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under grant Nos. ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Program (FP7/2007–2013), including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq grant 465376/2014-2).
Published: 2022

16. Dark Energy Survey Year 3 results: Cosmology with moments of weak lensing mass maps

Author: Gatti, M., Jain, B., Chang, C., Raveri, M., Zürcher, D., Secco, L., Whiteway, L., Jeffrey, N., Doux, C., Kacprzak, T., Bacon, D., Fosalba, P., Alarcon, A., Amon, A., Bechtol, K., Becker, M., Bernstein, G., Blazek, J., Campos, A., Choi, A., Davis, C., Derose, J., Dodelson, S., Elsner, F., Elvin-Poole, J., Everett, S., Ferte, A., Gruen, D., Harrison, I., Huterer, D., Jarvis, M., Krause, E., Leget, P. F., Lemos, P., Maccrann, N., Mccullough, J., Muir, J., Myles, J., Navarro, A., Pandey, S., Prat, J., Rollins, R. P., Roodman, A., Sanchez, C., Sheldon, E., Shin, T., Troxel, M., Tutusaus, I., Yin, B., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Cawthon, R., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Drlica-Wagner, A., Eckert, K., Evrard, A. E., Ferrero, I., García-Bellido, J., Gaztanaga, E., Giannantonio, T., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lahav, O., Lidman, C., Maia, M. A. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Palmese, A., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A. A., Reil, K., Rodriguez-Monroyv, M., Romer, A. K., Sanchez, E., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., DES Collaboration, Gatti, M., Jain, B., Chang, C., Raveri, M., Zürcher, D., Secco, L., Whiteway, L., Jeffrey, N., Doux, C., Kacprzak, T., Bacon, D., Fosalba, P., Alarcon, A., Amon, A., Bechtol, K., Becker, M., Bernstein, G., Blazek, J., Campos, A., Choi, A., Davis, C., Derose, J., Dodelson, S., Elsner, F., Elvin-Poole, J., Everett, S., Ferte, A., Gruen, D., Harrison, I., Huterer, D., Jarvis, M., Krause, E., Leget, P. F., Lemos, P., Maccrann, N., Mccullough, J., Muir, J., Myles, J., Navarro, A., Pandey, S., Prat, J., Rollins, R. P., Roodman, A., Sanchez, C., Sheldon, E., Shin, T., Troxel, M., Tutusaus, I., Yin, B., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Cawthon, R., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Drlica-Wagner, A., Eckert, K., Evrard, A. E., Ferrero, I., García-Bellido, J., Gaztanaga, E., Giannantonio, T., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lahav, O., Lidman, C., Maia, M. A. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Palmese, A., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A. A., Reil, K., Rodriguez-Monroyv, M., Romer, A. K., Sanchez, E., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., Des, Collaboration, UAM. Departamento de Física Teórica, Ministerio de Ciencia, Innovación y Universidades (España), European Research Council, European Commission, Agencia Estatal de Investigación (España), Generalitat de Catalunya, Ministerio de Economía y Competitividad (España), Department of Energy (US), National Aeronautics and Space Administration (US), and National Science Foundation (US)
Subjects: Gravitational Lensing, data-compression, inference, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Física, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, parameter-estimation, universe, Dark Energy, Astrophysic, cosmic shear 2-point, model predictions, galaxy, simulations, Weak, peak statistics, constraints, Cosmology and Nongalactic Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: DES Collaboration: M. Gatti et al., We present a cosmological analysis using the second and third moments of the weak lensing mass (convergence) maps from the first three years of data (Y3) data of the Dark Energy Survey. The survey spans an effective area of 4139 square degrees and uses the images of over 100 million galaxies to reconstruct the convergence field. The second moment of the convergence as a function of smoothing scale contains information similar to standard shear 2-point statistics. The third moment, or the skewness, contains additional non-Gaussian information. The data is analyzed in the context of the ΛCDM model, varying five cosmological parameters and 19 nuisance parameters modeling astrophysical and measurement systematics. Our modeling of the observables is completely analytical, and has been tested with simulations in our previous methodology study. We obtain a 1.7% measurement of the amplitude of fluctuations parameter S8≡σ8(Ωm/0.3)0.5=0.784±0.013. The measurements are shown to be internally consistent across redshift bins, angular scales, and between second and third moments. In particular, the measured third moment is consistent with the expectation of gravitational clustering under the ΛCDM model. The addition of the third moment improves the constraints on S8 and Ωm by ∼15% and ∼25% compared to an analysis that only uses second moments. We compare our results with Planck constraints from the cosmic microwave background, finding a 2.2–2.8σ tension in the full parameter space, depending on the combination of moments considered. The third moment, independently, is in 2.8σ tension with Planck, and thus provides a cross-check on the analyses of 2-point correlations., Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministerio da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciencies de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, NSF’s NOIRLab, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. Based in part on observations at Cerro Tololo Inter-American Observatory at NSF’s NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under Grants No. AST-1138766 and No. AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under Grants No. ESP2017-89838, No. PGC2018-094773, No. PGC2018-102021, No. SEV-2016-0588, No. SEV-2016-0597, and No. MDM-2015-0509, some of which include ERDF funds from the European Union. I. F. A. E. is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC Grant agreements No. 240672, No. 291329, and No. 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq Grant No. 465376/2014-2). This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DEAC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics.
Published: 2022

17. Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing

Author: DES Collaboration, Abbott, T. M. C., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Andrade-Oliveira, F., Annis, J., Avila, S., Bacon, D., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Bhargava, S., Birrer, S., Blazek, J., Brandao-Souza, A., Bridle, S. L., Brooks, D., Buckley-Geer, E., Burke, D. L., Camacho, H., Campos, A., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F. J., Cawthon, R., Chang, C., Chen, A., Chen, R., Choi, A., Conselice, C., Cordero, J., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. da Silva, Davis, C., Davis, T. M., De Vicente, J., DeRose, J., Desai, S., Di Valentino, E., Diehl, H. T., Dietrich, J. P., Dodelson, S., Doel, P., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Elvin-Poole, J., Everett, S., Evrard, A. E., Fang, X., Farahi, A., Fernandez, E., Ferrero, I., Fert��, A., Fosalba, P., Friedrich, O., Frieman, J., Garc��a-Bellido, J., Gatti, M., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Giannini, G., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Harrison, I., Hartley, W. G., Herner, K., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., Huff, E. M., Huterer, D., Jain, B., James, D. J., Jarvis, M., Jeffrey, N., Jeltema, T., Kovacs, A., Krause, E., Kron, R., Kuehn, K., Kuropatkin, N., Lahav, O., Leget, P. -F., Lemos, P., Liddle, A. R., Lidman, C., Lima, M., Lin, H., MacCrann, N., Maia, M. A. G., Marshall, J. L., Martini, P., McCullough, J., Melchior, P., Mena-Fern��ndez, J., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Muir, J., Myles, J., Nadathur, S., Navarro-Alsina, A., Nichol, R. C., Ogando, R. L. C., Omori, Y., Palmese, A., Pandey, S., Park, Y., Paz-Chinch��n, F., Petravick, D., Pieres, A., Malag��n, A. A. Plazas, Porredon, A., Prat, J., Raveri, M., Rodriguez-Monroy, M., Rollins, R. P., Romer, A. K., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., S��nchez, C., Sanchez, E., Sanchez, J., Cid, D. Sanchez, Scarpine, V., Schubnell, M., Scolnic, D., Secco, L. F., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tabbutt, M., Tarle, G., Thomas, D., To, C., Troja, A., Troxel, M. A., Tucker, D. L., Tutusaus, I., Varga, T. N., Walker, A. R., Weaverdyck, N., Wechsler, R., Weller, J., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Abbott, T. M. C., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Andrade-Oliveira, F., Annis, J., Avila, S., Bacon, D., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Bhargava, S., Birrer, S., Blazek, J., Brandao-Souza, A., Bridle, S. L., Brooks, D., Buckley-Geer, E., Burke, D. L., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Cawthon, R., Chang, C., Chen, A., Chen, R., Choi, A., Conselice, C., Cordero, J., Costanzi, M., Crocce, M., Da Costa, L. N., Da Silva Pereira, M. E., Davis, C., Davis, T. M., De Vicente, J., Derose, J., Desai, S., Di Valentino, E., Diehl, H. T., Dietrich, J. P., Dodelson, S., Doel, P., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Elvin-Poole, J., Everett, S., Evrard, A. E., Fang, X., Farahi, A., Fernandez, E., Ferrero, I., Ferte, A., Fosalba, P., Friedrich, O., Frieman, J., Garcia-Bellido, J., Gatti, M., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Giannini, G., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Harrison, I., Hartley, W. G., Herner, K., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., Huff, E. M., Huterer, D., Jain, B., James, D. J., Jarvis, M., Jeffrey, N., Jeltema, T., Kovacs, A., Krause, E., Kron, R., Kuehn, K., Kuropatkin, N., Lahav, O., Leget, P. -F., Lemos, P., Liddle, A. R., Lidman, C., Lima, M., Lin, H., Maccrann, N., Maia, M. A. G., Marshall, J. L., Martini, P., Mccullough, J., Melchior, P., Mena-Fernandez, J., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Muir, J., Myles, J., Nadathur, S., Navarro-Alsina, A., Nichol, R. C., Ogando, R. L. C., Omori, Y., Palmese, A., Pandey, S., Park, Y., Paz-Chinchon, F., Petravick, D., Pieres, A., Plazas Malagon, A. A., Porredon, A., Prat, J., Raveri, M., Rodriguez-Monroy, M., Rollins, R. P., Romer, A. K., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sanchez, C., Sanchez, E., Sanchez, J., Sanchez Cid, D., Scarpine, V., Schubnell, M., Scolnic, D., Secco, L. F., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tabbutt, M., Tarle, G., Thomas, D., To, C., Troja, A., Troxel, M. A., Tucker, D. L., Tutusaus, I., Varga, T. N., Walker, A. R., Weaverdyck, N., Wechsler, R., Weller, J., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Ministerio de Ciencia, Innovación y Universidades (España), European Research Council, European Commission, Agencia Estatal de Investigación (España), Ministerio de Economía y Competitividad (España), Department of Energy (US), Generalitat de Catalunya, National Aeronautics and Space Administration (US), National Science Foundation (US), NSF's National Optical-Infrared Astronomy Research Laboratory, Laboratório Interinstitucional de E-Astronomia - LIneA, Argonne National Laboratory, Fermi National Accelerator Laboratory, University of Michigan, Universidade Estadual Paulista (UNESP), Stanford University, Universidad Autonoma de Madrid, University of Portsmouth, University of Hawai'i, University of Wisconsin-Madison, University of Pennsylvania, University of Sussex, 450 Serra Mall, Northeastern University, Observatoire de Sauverny, Universidade Estadual de Campinas (UNICAMP), University of Manchester, University College London, University of Chicago, SLAC National Accelerator Laboratory, Carnegie Mellon University, Instituto de Astrofisica de Canarias, Dpto. Astrofísica, National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign, The Barcelona Institute of Science and Technology, Institut d'Estudis Espacials de Catalunya (IEEC), Institute of Space Sciences (ICE CSIC), Duke University, The Ohio State University, School of Physics and Astronomy, University of Trieste, INAF-Osservatorio Astronomico di Trieste, Institute for Fundamental Physics of the Universe, Observatório Nacional, University of Queensland, Medioambientales y Tecnológicas (CIEMAT), Lawrence Berkeley National Laboratory, IIT Hyderabad, Ludwig-Maximilians-Universität, University of Arizona, California Institute of Technology, Santa Cruz Institute for Particle Physics, University of Texas at Austin, University of Oslo, University of Cambridge, 382 Via Pueblo Mall, Denys Wilkinson Building, University of Geneva, Center for Astrophysics and Harvard and Smithsonian, Université de Paris, Macquarie University, Lowell Observatory, University of Edinburgh, Universidade de Lisboa, Perimeter Institute for Theoretical Physics, The Australian National University, Australian National University, Universidade de São Paulo (USP), Texas AandM University, Harvard University, Peyton Hall, Institució Catalana de Recerca i Estudis Avançats, Max Planck Institute for Extraterrestrial Physics, The University of Tokyo, Brookhaven National Laboratory, University of Southampton, Oak Ridge National Laboratory, Ludwig-Maximilians Universität München, Laboratoire de physique de l'ENS - ENS Paris (LPENS (UMR_8023)), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), DES, UAM. Departamento de Física Teórica, Laboratoire de physique de l'ENS - ENS Paris (LPENS), Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Sorbonne Université (SU)-École normale supérieure - Paris (ENS Paris), and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)
Subjects: luminous red galaxies, Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, parameter constraints, supernova legacy survey, Astrophysics, 01 natural sciences, Astrophysic, Cosmology and Nongalactic Astrophysics, 0103 physical sciences, LENTES GRAVITACIONAIS, Weak, 010303 astronomy & astrophysics, mass correlation-function, Gravitational Lensing, extragalactic objects, 010308 nuclear & particles physics, Física, Dark Energy, ia supernovae, digital sky survey, power-spectrum, photometric data set, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], cosmic shear, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: DES Collaboration: T. M. C. Abbott et al., We present the first cosmology results from large-scale structure using the full 5000 deg2 of imaging data from the Dark Energy Survey (DES) Data Release 1. We perform an analysis of large-scale structure combining three two-point correlation functions (3×2pt): (i) cosmic shear using 100 million source galaxies, (ii) galaxy clustering, and (iii) the cross-correlation of source galaxy shear with lens galaxy positions, galaxy–galaxy lensing. To achieve the cosmological precision enabled by these measurements has required updates to nearly every part of the analysis from DES Year 1, including the use of two independent galaxy clustering samples, modeling advances, and several novel improvements in the calibration of gravitational shear and photometric redshift inference. The analysis was performed under strict conditions to mitigate confirmation or observer bias; we describe specific changes made to the lens galaxy sample following unblinding of the results and tests of the robustness of our results to this decision. We model the data within the flat ΛCDM and wCDM cosmological models, marginalizing over 25 nuisance parameters. We find consistent cosmological results between the three two-point correlation functions; their combination yields clustering amplitude S8=0.776+0.017−0.017 and matter density Ωm=0.339+0.032−0.031 in ΛCDM, mean with 68% confidence limits; S8=0.775+0.026−0.024, Ωm=0.352+0.035−0.041, and dark energy equation-of-state parameter w=−0.98+0.32−0.20 in wCDM. These constraints correspond to an improvement in signal-to-noise of the DES Year 3 3×2pt data relative to DES Year 1 by a factor of 2.1, about 20% more than expected from the increase in observing area alone. This combination of DES data is consistent with the prediction of the model favored by the Planck 2018 cosmic microwave background (CMB) primary anisotropy data, which is quantified with a probability-to-exceed p=0.13–0.48. We find better agreement between DES 3×2pt and Planck than in DES Y1, despite the significantly improved precision of both. When combining DES 3×2pt data with available baryon acoustic oscillation, redshift-space distortion, and type Ia supernovae data, we find p=0.34. Combining all of these datasets with Planck CMB lensing yields joint parameter constraints of S8=0.812+0.008−0.008, Ωm=0.306+0.004−0.005, h=0.680+0.004−0.003, and ∑mν, Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministerio da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ci`encies de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, NFS’s NOIRLab, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. Based in part on observations at Cerro Tololo Inter-American Observatory at NSF’s NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under Grants No. AST-1138766 and No. AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under grants No. ESP2017-89838, No. PGC2018-094773, No. PGC2018-102021, No. SEV-2016-0588, No. SEV-2016-0597, and No. MDM-2015-0509, some of which include ERDF funds from the European Union. I. F. A. E. E. is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC grant agreements No. 240672, No. 291329, and No. 306478.We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq grant No. 465376/2014-2). This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics. This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. This work also used resources on Duke Compute Cluster (DCC), the CCAPP condo of the Ruby Cluster at the Ohio Supercomputing Center [232], and computing resources at SLAC National Accelerator Laboratory. We also thank the staff of the Fermilab Computing Sector for their support. Plots in this manuscript were produced partly with MATPLOTLIB [233], and it has been prepared using NASA’s Astrophysics Data System Bibliographic Services.
Published: 2022

18. Nationwide multidisciplinary consensus on the clinical management of Merkel cell carcinoma: a Delphi panel

Author: Spada F., Bossi P., Caraco C., Sileni V. C., Dei Tos A. P., Fazio N., Grignani G., Maio M., Quaglino P., Queirolo P., Ascierto P. A., Antonini Cappellini G. C., Antonuzzo L., Badalamenti G., Barberis M., Bassetto F., Berardi R., Berruti A., Bongiovanni A., Bonomo P., Borgognoni L., Borzillo V., Bruder F., Campana D., Consoli F., Cordova A., Depenni R., Di Giacomo A. M., Fabbrocini G., Fargnoli M. C., Ferraresi V., Ferrau F., Fierro M. T., Gatti M., Gelsomino F., Giuffrida D., Graziano P., Gregorelli C., Guida M., Massi D., Mazzarotto R., Milesi L., Minisini A. M., Morgese F., Muto P., Palmieri G., Patuzzo R., Pellacani G., Picciotto F., Pigozzo J., Pimpinelli N., Poletti P., Repetto L., Rinaldi G., Rubegni P., Rubino G., Spagnolo F., Tagliaferri L., Tanda E., Tronconi M. C., Tucci M., Valente M., Vincenzi B., Zalaudek I., Spada F., Bossi P., Caraco C., Sileni V.C., Dei Tos A.P., Fazio N., Grignani G., Maio M., Quaglino P., Queirolo P., Ascierto P.A., Antonini Cappellini G.C., Antonuzzo L., Badalamenti G., Barberis M., Bassetto F., Berardi R., Berruti A., Bongiovanni A., Bonomo P., Borgognoni L., Borzillo V., Bruder F., Campana D., Consoli F., Cordova A., Depenni R., Di Giacomo A.M., Fabbrocini G., Fargnoli M.C., Ferraresi V., Ferrau F., Fierro M.T., Gatti M., Gelsomino F., Giuffrida D., Graziano P., Gregorelli C., Guida M., Massi D., Mazzarotto R., Milesi L., Minisini A.M., Morgese F., Muto P., Palmieri G., Patuzzo R., Pellacani G., Picciotto F., Pigozzo J., Pimpinelli N., Poletti P., Repetto L., Rinaldi G., Rubegni P., Rubino G., Spagnolo F., Tagliaferri L., Tanda E., Tronconi M.C., Tucci M., Valente M., Vincenzi B., and Zalaudek I.
Subjects: Pharmacology, Cancer Research, Skin Neoplasms, Immunology, Carcinoma, Carcinoma, Merkel Cell, Oncology, Italy, Merkel cell polyomavirus, Merkel Cell, Molecular Medicine, Immunology and Allergy, immunotherapy, radiotherapy, skin neoplasms, Humans, Immunotherapy
Abstract: Merkel cell carcinoma (MCC) is a rare and highly aggressive cutaneous neuroendocrine carcinoma. The MCC incidence rate has rapidly grown over the last years, with Italy showing the highest increase among European countries. This malignancy has been the focus of active scientific research over the last years, focusing mainly on pathogenesis, new therapeutic trials and diagnosis. A national expert board developed 28 consensus statements that delineated the evolution of disease management and highlighted the paradigm shift towards the use of immunological strategies, which were then presented to a national MCC specialists panel for review. Sixty-five panelists answered both rounds of the questionnaire. The statements were divided into five areas: a high level of agreement was reached in the area of guidelines and multidisciplinary management, even if in real life the multidisciplinary team was not always represented by all the specialists. In the diagnostic pathway area, imaging played a crucial role in diagnosis and initial staging, planning for surgery or radiation therapy, assessment of treatment response and surveillance of recurrence and metastases. Concerning diagnosis, the usefulness of Merkel cell polyomavirus is recognized, but the agreement and consensus regarding the need for cytokeratin evaluation appears greater. Regarding the areas of clinical management and follow-up, patients with MCC require customized treatment. There was a wide dispersion of results and the suggestion to increase awareness about the adjuvant radiation therapy. The panelists unanimously agreed that the information concerning avelumab provided by the JAVELIN Merkel 200 study is adequate and reliable and that the expanded access program data could have concrete clinical implications. An immunocompromised patient with advanced MCC can be treated with immunotherapy after multidisciplinary risk/benefit assessment, as evidenced by real-world analysis and highlighted in the guidelines. A very high consensus regarding the addition of radiotherapy to treat the ongoing focal progression of immunotherapy was observed. This paper emphasizes the importance of collaboration and communication among the interprofessional team members and encourages managing patients with MCC within dedicated multidisciplinary teams. New insights in the treatment of this challenging cancer needs the contribution of many and different experts.
Published: 2022

19. Dark energy survey year 3 results: High-precision measurement and modeling of galaxy-galaxy lensing

Author: Prat, J., Blazek, J., Sánchez, C., Tutusaus, I., Pandey, S., Elvin-Poole, J., Krause, E., Troxel, M. A., Secco, L. F., Amon, A., Derose, J., Zacharegkas, G., Chang, C., Jain, B., Maccrann, N., Park, Y., Sheldon, E., Giannini, G., Bocquet, S., To, C., Alarcon, A., Alves, O., Andrade-Oliveira, F., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Chen, R., Choi, A., Cordero, J., Crocce, M., Davis, C., De Vicente, J., Diehl, H. T., Dodelson, S., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Everett, S., Fang, X., Farahi, A., Ferté, A., Fosalba, P., Friedrich, O., Gatti, M., Gruen, D., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Huang, H., Huff, E. M., Huterer, D., Jarvis, M., Kuropatkin, N., Leget, P. -F., Lemos, P., Liddle, A. R., Mccullough, J., Muir, J., Myles, J., Navarro-Alsina, A., Porredon, A., Raveri, M., Rodriguez-Monroy, M., Rollins, R. P., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Sanchez, J., Sevilla-Noarbe, I., Shin, T., Troja, A., Varga, T. N., Weaverdyck, N., Wechsler, R. H., Yanny, B., Yin, B., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Bacon, D., Brooks, D., Burke, D. L., Carretero, J., Conselice, C., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Desai, S., Dietrich, J. P., Doel, P., Evrard, A. E., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., Lin, H., Maia, M. A. G., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miller, C. J., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Petravick, D., Plazas Malagón, A. A., Sanchez, E., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., Weller, J., Des, Collaboration, A Prat, J., Blazek, J., Sánchez, C., Tutusaus, I., Pandey, S., Elvin- Poole, J., Krause, E., Troxel, M. A., Secco, L. F., Amon, A., Derose, J., Zacharegkas, G., Chang, C., Jain, B., Maccrann, N., Park, Y., Sheldon, E., Giannini, G., Bocquet, S., To, C., Alarcon, A., Alves, O., Andrade-Oliveira, F., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Chen, R., Choi, A., Cordero, J., Crocce, M., Davis, C., De Vicente, J., Diehl, H. T., Dodelson, S., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Everett, S., Fang, X., Farahi, A., Ferté, A., Fosalba, P., Friedrich, O., Gatti, M., Gruen, D., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Huang, H., Huff, E. M., Huterer, D., Jarvis, M., Kuropatkin, N., Leget, P. -F., Lemos, P., Liddle, A. R., Mccullough, J., Muir, J., Myles, J., Navarro- Alsina, A., Porredon, A., Raveri, M., Rodriguez-Monroy, M., Rollins, R. P., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Sanchez, J., Sevilla-Noarbe, I., Shin, T., Troja, A., Varga, T. N., Weaverdyck, N., Wechsler, R. H., Yanny, B., Yin, B., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Bacon, D., Brooks, D., Burke, D. L., Carretero, J., Conselice, C., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Desai, S., Dietrich, J. P., Doel, P., Evrard, A. E., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Lahav, O., Lin, H., Maia, M. A. G., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miller, C. J., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Petravick, D., Plazas Malagón, A. A., Sanchez, E., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., Weller, J., and UAM. Departamento de Física Teórica
Subjects: Gravitational Lensing, Cosmology and Nongalactic Astrophysics (astro-ph.CO), cosmological parameter constraints, FOS: Physical sciences, Física, marginalization, Astrophysics::Cosmology and Extragalactic Astrophysics, calibration, Astrophysics, Dark Energy, Astrophysic, Cosmology and Nongalactic Astrophysics, redshift distribution, mass, Weak, photometric data set, sdss, cosmic shear, Astrophysics - Cosmology and Nongalactic Astrophysics, intrinsic alignments
Abstract: DES Collaboration: J. Prat et al., We present and characterize the galaxy-galaxy lensing signal measured using the first three years of data from the Dark Energy Survey (DES Y3) covering 4132 deg2. These galaxy-galaxy measurements are used in the DES Y3 3×2pt cosmological analysis, which combines weak lensing and galaxy clustering information. We use two lens samples: a magnitude-limited sample and the redmagic sample, which span the redshift range ∼0.2–1 with 10.7 and 2.6 M galaxies, respectively. For the source catalog, we use the metacalibration shape sample, consisting of ≃100M galaxies separated into four tomographic bins. Our galaxy-galaxy lensing estimator is the mean tangential shear, for which we obtain a total SNR of ∼148 for maglim (∼120 for redmagic), and ∼67 (∼55) after applying the scale cuts of 6Mpc/h. Thus we reach percent-level statistical precision, which requires that our modeling and systematic-error control be of comparable accuracy. The tangential shear model used in the 3×2pt cosmological analysis includes lens magnification, a five-parameter intrinsic alignment model, marginalization over a point mass to remove information from small scales and a linear galaxy bias model validated with higher-order terms. We explore the impact of these choices on the tangential shear observable and study the significance of effects not included in our model, such as reduced shear, source magnification, and source clustering. We also test the robustness of our measurements to various observational and systematics effects, such as the impact of observing conditions, lens-source clustering, random-point subtraction, scale-dependent metacalibration responses, point spread function residuals, and B modes.
Published: 2022

20. Robust sampling for weak lensing and clustering analyses with the dark energy survey

Author: Lemos, P., Weaverdyck, N., Rollins, R. P., Muir, J., Ferté, A., Liddle, A. R., Campos, A., Huterer, D., Raveri, M., Zuntz, J., Di Valentino, E., Fang, X., Hartley, W. G., Aguena, M., Allam, S., Annis, J., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Choi, A., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., Dietrich, J. P., Everett, S., Ferrero, I., Frieman, J., García-Bellido, J., Gatti, M., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lima, M., March, M., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Palmese, A., Paz-Chinchón, F., Pieres, A., Malagón, A. A. Plazas, Porredon, A., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J., DES Collaboration, Lemos, P., Weaverdyck, N., Rollins, R. P., Muir, J., Ferté, A., Liddle, A. R., Campos, A., Huterer, D., Raveri, M., Zuntz, J., Di Valentino, E., Fang, X., Hartley, W. G., Aguena, M., Allam, S., Annis, J., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Choi, A., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., Dietrich, J. P., Everett, S., Ferrero, I., Frieman, J., García-Bellido, J., Gatti, M., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lima, M., March, M., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Palmese, A., Paz-Chinchón, F., Pieres, A., Malagón, A. A. Plaza, Porredon, A., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J., and Des, Collaboration
Subjects: methods: statistical, Cosmology and Nongalactic Astrophysics (astro-ph.CO), statistical [methods], cosmological parameter [cosmology], FOS: Physical sciences, Astronomy and Astrophysics, cosmology: large-scale structure of the Universe, cosmology: cosmological parameters, cosmology: observations, Space and Planetary Science, large-scale structure of the Universe [cosmology], Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), observation [cosmology], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Recent cosmological analyses rely on the ability to accurately sample from high-dimensional posterior distributions. A variety of algorithms have been applied in the field, but justification of the particular sampler choice and settings is often lacking. Here we investigate three such samplers to motivate and validate the algorithm and settings used for the Dark Energy Survey (DES) analyses of the first 3 years (Y3) of data from combined measurements of weak lensing and galaxy clustering. We employ the full DES Year 1 likelihood alongside a much faster approximate likelihood, which enables us to assess the outcomes from each sampler choice and demonstrate the robustness of our full results. We find that the ellipsoidal nested sampling algorithm $\texttt{MultiNest}$ reports inconsistent estimates of the Bayesian evidence and somewhat narrower parameter credible intervals than the sliced nested sampling implemented in $\texttt{PolyChord}$. We compare the findings from $\texttt{MultiNest}$ and $\texttt{PolyChord}$ with parameter inference from the Metropolis-Hastings algorithm, finding good agreement. We determine that $\texttt{PolyChord}$ provides a good balance of speed and robustness, and recommend different settings for testing purposes and final chains for analyses with DES Y3 data. Our methodology can readily be reproduced to obtain suitable sampler settings for future surveys., 16 pages, 11 figures
Published: 2022

21. Cross-correlation of Dark Energy Survey Year 3 lensing data with ACT and Planck thermal Sunyaev-Zel'dovich effect observations. II. Modeling and constraints on halo pressure profiles

Author: A Pandey, S., Gatti, M., Baxter, E., Hill, J. C., Fang, X., Doux, C., Giannini, G., Raveri, M., Derose, J., Huang, H., Moser, E., Battaglia, N., Alarcon, A., Amon, A., Becker, M., Campos, A., Chang, C., Chen, R., Choi, A., Eckert, K., Elvin-Poole, J., Everett, S., Ferte, A., Harrison, I., Maccrann, N., Mccullough, J., Myles, J., Navarro Alsina, A., Prat, J., Rollins, R. P., Sanchez, C., Shin, T., Troxel, M., Tutusaus, I., Yin, B., Aguena, M., Allam, S., Andrade-Oliveira, F., Bernstein, G. M., Bertin, E., Bolliet, B., Bond, J. R., Brooks, D., Calabrese, E., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Cawthon, R., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Dunkley, J., Evrard, A. E., Ferraro, S., Ferrero, I., Flaugher, B., Fosalba, P., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Herner, K., Hincks, A. D., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hughes, J. P., Huterer, D., Jain, B., James, D. J., Jeltema, T., Krause, E., Kuehn, K., Lahav, O., Lima, M., Lokken, M., Madhavacheril, M. S., Maia, M. A. G., Mcmahon, J. J., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Moodley, K., Morgan, R., Nati, F., Niemack, M. D., Page, L., Palmese, A., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A. A., Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Scarpine, V., Schaan, E., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Sherwin, B. D., Sifón, C., Smith, M., Soares-Santos, M., Spergel, D., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J., Wollack, E. J., Xu, Z., Des, Act, Collaboration, A Pandey, S., Gatti, M., Baxter, E., Hill, J. C., Fang, X., Doux, C., Giannini, G., Raveri, M., Derose, J., Huang, H., Moser, E., Battaglia, N., Alarcon, A., Amon, A., Becker, M., Campos, A., Chang, C., Chen, R., Choi, A., Eckert, K., Elvin-Poole, J., Everett, S., Ferte, A., Harrison, I., Maccrann, N., Mccullough, J., Myles, J., Navarro Alsina, A., Prat, J., Rollins, R. P., Sanchez, C., Shin, T., Troxel, M., Tutusaus, I., Yin, B., Aguena, M., Allam, S., Andrade-Oliveira, F., Bernstein, G. M., Bertin, E., Bolliet, B., Bond, J. R., Brooks, D., Calabrese, E., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Cawthon, R., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Dunkley, J., Evrard, A. E., Ferraro, S., Ferrero, I., Flaugher, B., Fosalba, P., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Herner, K., Hincks, A. D., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hughes, J. P., Huterer, D., Jain, B., James, D. J., Jeltema, T., Krause, E., Kuehn, K., Lahav, O., Lima, M., Lokken, M., Madhavacheril, M. S., Maia, M. A. G., Mcmahon, J. J., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Moodley, K., Morgan, R., Nati, F., Niemack, M. D., Page, L., Palmese, A., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A. A., Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Scarpine, V., Schaan, E., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Sherwin, B. D., Sifón, C., Smith, M., Soares-Santos, M., Spergel, D., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J., Wollack, E. J., Xu, Z., Des, and Act, Collaboration
Subjects: Astrophysic, Astrophysics, Cosmology and Nongalactic Astrophysics
Abstract: Hot, ionized gas leaves an imprint on the cosmic microwave background via the thermal Sunyaev-Zel'dovich (tSZ) effect. The cross-correlation of gravitational lensing (which traces the projected mass) with the tSZ effect (which traces the projected gas pressure) is a powerful probe of the thermal state of ionized baryons throughout the Universe and is sensitive to effects such as baryonic feedback. In a companion paper (Gatti et al. Phys. Rev. D 105, 123525 (2022)PRVDAQ2470-0010), we present tomographic measurements and validation tests of the cross-correlation between Galaxy shear measurements from the first three years of observations of the Dark Energy Survey and tSZ measurements from a combination of Atacama Cosmology Telescope and Planck observations. In this work, we use the same measurements to constrain models for the pressure profiles of halos across a wide range of halo mass and redshift. We find evidence for reduced pressure in low-mass halos, consistent with predictions for the effects of feedback from active Galactic nuclei. We infer the hydrostatic mass bias (BM500c/MSZ) from our measurements, finding B=1.8±0.1 when adopting the Planck-preferred cosmological parameters. We additionally find that our measurements are consistent with a nonzero redshift evolution of B, with the correct sign and sufficient magnitude to explain the mass bias necessary to reconcile cluster count measurements with the Planck-preferred cosmology. Our analysis introduces a model for the impact of intrinsic alignments (IAs) of galaxy shapes on the shear-tSZ correlation. We show that IA can have a significant impact on these correlations at current noise levels.
Published: 2022

22. Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and galaxy-galaxy lensing using the MagLim lens sample

Author: Porredon, A., Crocce, M., Elvin-Poole, J., Cawthon, R., Giannini, G., De Vicente, J., Carnero Rosell, A., Ferrero, I., Krause, E., Fang, X., Prat, J., Rodriguez-Monroy, M., Pandey, S., Pocino, A., Castander, F. J., Choi, A., Amon, A., Tutusaus, I., Dodelson, S., Sevilla-Noarbe, I., Fosalba, P., Gaztanaga, E., Alarcon, A., Alves, O., Andrade-Oliveira, F., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Blazek, J., Camacho, H., Campos, A., Carrasco Kind, M., Chintalapati, P., Cordero, J., Derose, J., Di Valentino, E., Doux, C., Eifler, T. F., Everett, S., Ferté, A., Friedrich, O., Gatti, M., Gruen, D., Harrison, I., Hartley, W. G., Herner, K., Huff, E. M., Huterer, D., Jain, B., Jarvis, M., Lee, S., Lemos, P., Maccrann, N., Mena-Fernández, J., Muir, J., Myles, J., Park, Y., Raveri, M., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, E., Sanchez, J., Sanchez Cid, D., Scolnic, D., Secco, L. F., Sheldon, E., Troja, A., Troxel, M. A., Weaverdyck, N., Yanny, B., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Avila, S., Bacon, D., Bertin, E., Bhargava, S., Brooks, D., Buckley-Geer, E., Burke, D. L., Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Davis, T. M., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Drlica-Wagner, A., Eckert, K., Evrard, A. E., Flaugher, B., Frieman, J., García-Bellido, J., Gerdes, D. W., Giannantonio, T., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Kuehn, K., Kuropatkin, N., Lahav, O., Lidman, C., Lima, M., Lin, H., Maia, M. A. G., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Petravick, D., Pieres, A., Plazas Malagón, A. A., Romer, A. K., Santiago, B., Scarpine, V., Schubnell, M., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J., Des, Collaboration, Ministerio de Ciencia, Innovación y Universidades (España), Agencia Estatal de Investigación (España), European Commission, Generalitat de Catalunya, European Research Council, Department of Energy (US), National Science Foundation (US), National Aeronautics and Space Administration (US), Porredon, A., Crocce, M., Elvin-Poole, J., Cawthon, R., Giannini, G., De Vicente, J., Carnero Rosell, A., Ferrero, I., Krause, E., Fang, X., Prat, J., Rodriguez-Monroy, M., Pandey, S., Pocino, A., Castander, F. J., Choi, A., Amon, A., Tutusaus, I., Dodelson, S., Sevilla-Noarbe, I., Fosalba, P., Gaztanaga, E., Alarcon, A., Alves, O., Andrade-Oliveira, F., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Blazek, J., Camacho, H., Campos, A., Carrasco Kind, M., Chintalapati, P., Cordero, J., Derose, J., Di Valentino, E., Doux, C., Eifler, T. F., Everett, S., Ferté, A., Friedrich, O., Gatti, M., Gruen, D., Harrison, I., Hartley, W. G., Herner, K., Huff, E. M., Huterer, D., Jain, B., Jarvis, M., Lee, S., Lemos, P., Maccrann, N., Mena-Fernández, J., Muir, J., Myles, J., Park, Y., Raveri, M., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, E., Sanchez, J., Sanchez Cid, D., Scolnic, D., Secco, L. F., Sheldon, E., Troja, A., Troxel, M. A., Weaverdyck, N., Yanny, B., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Avila, S., Bacon, D., Bertin, E., Bhargava, S., Brooks, D., Buckley-Geer, E., Burke, D. L., Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Davis, T. M., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Drlica-Wagner, A., Eckert, K., Evrard, A. E., Flaugher, B., Frieman, J., García-Bellido, J., Gerdes, D. W., Giannantonio, T., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Kuehn, K., Kuropatkin, N., Lahav, O., Lidman, C., Lima, M., Lin, H., Maia, M. A. G., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Petravick, D., Pieres, A., Plazas Malagón, A. A., Romer, A. K., Santiago, B., Scarpine, V., Schubnell, M., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J., Des, Collaboration, HEP, INSPIRE, Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), and DES
Subjects: luminous red galaxies, data release, pau survey, Cosmology and Nongalactic Astrophysics (astro-ph.CO), roman-space-telescope, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, oscillation spectroscopic survey, Astrophysic, Cosmology and Nongalactic Astrophysics, internal consistency, digital sky survey, redshift distributions, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], photometric data set, [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], cosmic shear, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: DES Collaboration: A. Porredon et al., The cosmological information extracted from photometric surveys is most robust when multiple probes of the large scale structure of the Universe are used. Two of the most sensitive probes are the clustering of galaxies and the tangential shear of background galaxy shapes produced by those foreground galaxies, so-called galaxy-galaxy lensing. Combining the measurements of these two two-point functions leads to cosmological constraints that are independent of the way galaxies trace matter (the galaxy bias factor). The optimal choice of foreground, or lens, galaxies is governed by the joint, but conflicting requirements to obtain accurate redshift information and large statistics. We present cosmological results from the full 5000deg2 of the Dark Energy Survey’s first three years of observations (Y3) combining those two-point functions, using for the first time a magnitude-limited lens sample (MagLim) of 11 million galaxies, especially selected to optimize such combination, and 100 million background shapes. We consider two flat cosmological models, the Standard Model with dark energy and cold dark matter (ΛCDM ) a variation with a free parameter for the dark energy equation of state (wCDM). Both models are marginalized over 25 astrophysical and systematic nuisance parameters. In ΛCDM we obtain for the matter density Ωm=0.320+0.041−0.034 and for the clustering amplitude S8≡σ8(Ωm/0.3)0.5=0.778+0.037−0.031, at 68% C.L. The latter is only 1σ smaller than the prediction in this model informed by measurements of the cosmic microwave background by the Planck satellite. In wCDM we find Ωm=0.32+0.044−0.046, S8=0.777+0.049−0.051 and dark energy equation of state w=−1.031+0.218−0.379. We find that including smaller scales, while marginalizing over nonlinear galaxy bias, improves the constraining power in the Ωm−S8 plane by 31% and in the Ωm−w plane by 41% while yielding consistent cosmological parameters from those in the linear bias case. These results are combined with those from cosmic shear in a companion paper to present full DES-Y3 constraints from the three two-point functions (3×2pt)., Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministerio da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciencies de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. Based in part on observations at Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management systemis supported by the National Science Foundation under Grants No. AST-1138766 and No. AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under Grants No. AYA2015-71825, No. ESP2015-66861, No. FPA2015-68048, No. SEV-2016-0588, No. SEV-2016-0597, and No. MDM-2015-0509, some of which include ERDF funds fromthe European Union. I. F. A. E. is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC Grant Agreements No. 240672, No. 291329, and No. 306478. We acknowledge support from the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through Project No. CE110001020, and the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) e-Universe (CNPq Grant No. 465376/2014-2). This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DEAC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics. The United States Government retains and the publisher, by accepting the article for publication, acknowledges that the United States Government retains a nonexclusive paid-up irrevocable world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes. Computations were made on the supercomputer Guillimin from McGill University, managed by Calcul Quebec and Compute Canada. The operation of this supercomputer is funded by the Canada Foundation for Innovation (CFI), the ministere de l’Économie, de la science et de l’innovation du Quebec (MESI) and the Fonds de recherche du Quebec-Nature et technologies (FRQ-NT). This research is part of the Blue Waters sustained-petascale computing project, which is supported by the National Science Foundation (Grants No. OCI-0725070 and No. ACI-1238993) and the state of Illinois. Blue Waters is a joint effort of the University of Illinois at Urbana-Champaign and its National Center for Supercomputing Applications. This research used resources of the Ohio Supercomputer Center (OSC) [117] and of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231.
Published: 2022

23. Core-collapse Supernovae in the Dark Energy Survey: Luminosity Functions and Host Galaxy Demographics

Author: Grayling, M., Gutiérrez, C. P., Sullivan, M., Wiseman, P., Vincenzi, M., Galbany, L., Möller, A., Brout, D., Davis, T. M., Frohmaier, C., Graur, O., Kelsey, L., Lidman, C., Popovic, B., Smith, M., Toy, M., Tucker, B. E., Zontou, Z., Abbott, T. M. C., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Asorey, J., Bacon, D., Bertin, E., Bocquet, S., Brooks, D., Rosell, A. Carnero, Carollo, D., Kind, M. Carrasco, Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Diehl, H. T., Doel, P., Everett, S., Ferrero, I., Friedel, D., Frieman, J., García-Bellido, J., Gatti, M., Gruen, D., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., Lewis, G. F., Malik, U., March, M., Menanteau, F., Miquel, R., Morgan, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Pieres, A., Malagón, A. A. Plazas, Rodriguez-Monroy, M., Romer, A. K., Roodman, A., Sanchez, E., Scarpine, V., Sevilla-Noarbe, I., Suchyta, E., Tarle, G., To, C., Tucker, D. L., and Varga, T. N.
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Space and Planetary Science, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Solar and Stellar Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics::Galaxy Astrophysics
Abstract: We present the luminosity functions and host galaxy properties of the Dark Energy Survey (DES) core-collapse supernova (CCSN) sample, consisting of 69 Type II and 50 Type Ibc spectroscopically and photometrically-confirmed supernovae over a redshift range $0.045, Comment: 28 pages, 13 figures, 5 tables. Accepted by MNRAS Dec 2022
Published: 2022

24. Dark Energy Survey Year 3 Results: Constraints on extensions to $\Lambda$CDM with weak lensing and galaxy clustering

Author: DES Collaboration, Abbott, T. M. C., Aguena, M., Alarcon, A., Alves, O., Amon, A., Annis, J., Avila, S., Bacon, D., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Birrer, S., Blazek, J., Bocquet, S., Brandao-Souza, A., Bridle, S. L., Brooks, D., Burke, D. L., Camacho, H., Campos, A., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F. J., Cawthon, R., Chang, C., Chen, A., Chen, R., Choi, A., Conselice, C., Cordero, J., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., Davis, C., Davis, T. M., DeRose, J., Desai, S., Di Valentino, E., Diehl, H. T., Dodelson, S., Doel, P., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Elvin-Poole, J., Everett, S., Fang, X., Farahi, A., Ferrero, I., Ferté, A., Flaugher, B., Fosalba, P., Friedel, D., Friedrich, O., Frieman, J., García-Bellido, J., Gatti, M., Giani, L., Giannantonio, T., Giannini, G., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hamaus, N., Harrison, I., Hartley, W. G., Herner, K., Hinton, S. R., Hollowood, D. L., Honscheid, K., Huang, H., Huff, E. M., Huterer, D., Jain, B., James, D. J., Jarvis, M., Jeffrey, N., Jeltema, T., Kovacs, A., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lee, S., Leget, P. -F., Lemos, P., Leonard, C. D., Liddle, A. R., Lima, M., Lin, H., MacCrann, N., Marshall, J. L., McCullough, J., Mena-Fernández, J., Menanteau, F., Miquel, R., Miranda, V., Mohr, J. J., Muir, J., Myles, J., Nadathur, S., Navarro-Alsina, A., Nichol, R. C., Ogando, R. L. C., Omori, Y., Palmese, A., Pandey, S., Park, Y., Paterno, M., Paz-Chinchón, F., Percival, W. J., Pieres, A., Malagón, A. A. Plazas, Porredon, A., Prat, J., Raveri, M., Rodriguez-Monroy, M., Rogozenski, P., Rollins, R. P., Romer, A. K., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, E., Sanchez, J., Cid, D. Sanchez, Scarpine, V., Scolnic, D., Secco, L. F., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Smith, M., Soares-Santos, M., Suchyta, E., Tabbutt, M., Tarle, G., Thomas, D., To, C., Troja, A., Troxel, M. A., Tutusaus, I., Varga, T. N., Vincenzi, M., Walker, A. R., Weaverdyck, N., Wechsler, R. H., Weller, J., Yanny, B., Yin, B., Zhang, Y., and Zuntz, J.
Subjects: Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We constrain extensions to the $\Lambda$CDM model using measurements from the Dark Energy Survey's first three years of observations and external data. The DES data are the two-point correlation functions of weak gravitational lensing, galaxy clustering, and their cross-correlation. We use simulated data and blind analyses of real data to validate the robustness of our results. In many cases, constraining power is limited by the absence of nonlinear predictions that are reliable at our required precision. The models are: dark energy with a time-dependent equation of state, non-zero spatial curvature, sterile neutrinos, modifications of gravitational physics, and a binned $\sigma_8(z)$ model which serves as a probe of structure growth. For the time-varying dark energy equation of state evaluated at the pivot redshift we find $(w_{\rm p}, w_a)= (-0.99^{+0.28}_{-0.17},-0.9\pm 1.2)$ at 68% confidence with $z_{\rm p}=0.24$ from the DES measurements alone, and $(w_{\rm p}, w_a)= (-1.03^{+0.04}_{-0.03},-0.4^{+0.4}_{-0.3})$ with $z_{\rm p}=0.21$ for the combination of all data considered. Curvature constraints of $\Omega_k=0.0009\pm 0.0017$ and effective relativistic species $N_{\rm eff}=3.10^{+0.15}_{-0.16}$ are dominated by external data. For massive sterile neutrinos, we improve the upper bound on the mass $m_{\rm eff}$ by a factor of three compared to previous analyses, giving 95% limits of $(\Delta N_{\rm eff},m_{\rm eff})\leq (0.28, 0.20\, {\rm eV})$. We also constrain changes to the lensing and Poisson equations controlled by functions $\Sigma(k,z) = \Sigma_0 \Omega_{\Lambda}(z)/\Omega_{\Lambda,0}$ and $\mu(k,z)=\mu_0 \Omega_{\Lambda}(z)/\Omega_{\Lambda,0}$ respectively to $\Sigma_0=0.6^{+0.4}_{-0.5}$ from DES alone and $(\Sigma_0,\mu_0)=(0.04\pm 0.05,0.08^{+0.21}_{-0.19})$ for the combination of all data. Overall, we find no significant evidence for physics beyond $\Lambda$CDM., Comment: Updated to match published version. 46 pages, 25 figures, data available at https://dev.des.ncsa.illinois.edu/releases/y3a2/Y3key-extensions
Published: 2022

25. Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approach

Author: Zürcher, D., Fluri, J., Sgier, R., Kacprzak, T., Gatti, M., Doux, C., Whiteway, L., Réfrégier, A., Chang, C., Jeffrey, N., Jain, B., Lemos, P., Bacon, D., Alarcon, A., Amon, A., Bechtol, K., Becker, M., Bernstein, G., Campos, A., Chen, R., Choi, A., Davis, C., Derose, J., Dodelson, S., Elsner, F., Elvin-Poole, J., Everett, S., Ferte, A., Gruen, D., Harrison, I., Huterer, D., Jarvis, M., Leget, P. F., MacCrann, N., McCullough, J., Muir, J., Myles, J., Navarro Alsina, A., Pandey, S., Prat, J., Raveri, M., Rollins, R. P., Roodman, A., Sanchez, C., Secco, L. F., Sheldon, E., Shin, T., Troxel, M., Tutusaus, I., Yin, B., Aguena, M., Allam, S., Andrade-Oliveira, F. [UNESP], Annis, J., Bertin, E., Brooks, D., Burke, D., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F., Cawthon, R., Conselice, C., Costanzi, M., Da Costa, L., Da Silva Pereira, M. E., Davis, T., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J., Doel, P., Eckert, K., Evrard, A., Ferrero, I., Flaugher, B., Fosalba, P., Friedel, D., Frieman, J., Garcia-Bellido, J., Gaztanaga, E., Gerdes, D., Giannantonio, T., Gruendl, R., Gschwend, J., Gutierrez, G., Hinton, S., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D., Kuehn, K., Kuropatkin, N., Lahav, O., Lidman, C., Lima, M., Maia, M., Marshall, J., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Palmese, A., Paz-Chinchon, F., Pieres, A., Plazas Malagón, A., Reil, K., Rodriguez Monroy, M., Romer, K., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla, I., Smith, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J., Wilkinson, R., National Science Foundation (US), Department of Energy (US), Swiss National Science Foundation, Ministerio de Educación y Ciencia (España), ETH Zurich, National Aeronautics and Space Administration (US), UAM. Departamento de Física Teórica, Zurcher, D., Fluri, J., Sgier, R., Kacprzak, T., Gatti, M., Doux, C., Whiteway, L., Refregier, A., Chang, C., Jeffrey, N., Jain, B., Lemos, P., Bacon, D., Alarcon, A., Amon, A., Bechtol, K., Becker, M., Bernstein, G., Campos, A., Chen, R., Choi, A., Davis, C., Derose, J., Dodelson, S., Elsner, F., Elvin-Poole, J., Everett, S., Ferte, A., Gruen, D., Harrison, I., Huterer, D., Jarvis, M., Leget, P. F., Maccrann, N., Mccullough, J., Muir, J., Myles, J., Navarro Alsina, A., Pandey, S., Prat, J., Raveri, M., Rollins, R. P., Roodman, A., Sanchez, C., Secco, L. F., Sheldon, E., Shin, T., Troxel, M., Tutusaus, I., Yin, B., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bertin, E., Brooks, D., Burke, D., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F., Cawthon, R., Conselice, C., Costanzi, M., Da Costa, L., Da Silva Pereira, M. E., Davis, T., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J., Doel, P., Eckert, K., Evrard, A., Ferrero, I., Flaugher, B., Fosalba, P., Friedel, D., Frieman, J., Garcia-Bellido, J., Gaztanaga, E., Gerdes, D., Giannantonio, T., Gruendl, R., Gschwend, J., Gutierrez, G., Hinton, S., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D., Kuehn, K., Kuropatkin, N., Lahav, O., Lidman, C., Lima, M., Maia, M., Marshall, J., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Palmese, A., Paz-Chinchon, F., Pieres, A., Plazas Malagon, A., Reil, K., Rodriguez Monroy, M., Romer, K., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla, I., Smith, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J., Wilkinson, R., Eth Zuurich, University of Pennsylvania, University College London, University of Chicago, University of Sussex, Université de Paris, University of Portsmouth, Argonne National Laboratory, Stanford University, University of WisconsinMadison, Carnegie Mellon University, Duke University, The Ohio State University, Lawrence Berkeley National Laboratory, Santa Cruz Institute for Particle Physics, California Institute of Technology, Ludwig-Maximilians-Universitat, Denys Wilkinson Building, University of Manchester, University of Michigan, University of Cambridge, Perimeter Institute for Theoretical Physics, 382 Via Pueblo Mall, Slac National Accelerator Laboratory, Universidade Estadual de Campinas (UNICAMP), Bldg 510, Institut d'Estudis Espacials de Catalunya (IEEC), CSIC), Laboratorio Interinstitucional de E-Astronomia-LIneA, Fermi National Accelerator Laboratory, Universidade Estadual Paulista (UNESP), Institut d'Astrophysique de Paris, National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign, The Barcelona Institute of Science and Technology, School of Physics and Astronomy, University of Trieste, INAF-Osservatorio Astronomico di Trieste, Institute for Fundamental Physics of the Universe, Observatorio Nacional, Universitat Hamburg, University of Queensland, Medioambientales y Tecnologicas (CIEMAT), Iit Hyderabad, University of Oslo, Universidad Autonoma de Madrid, Harvard and Smithsonian, Macquarie University, Lowell Observatory, The Australian National University, Australian National University, Universidade de São Paulo (USP), Texas A &m University, Peyton Hall, Institucio Catalana de Recerca i Estudis Avancats, 501 Campbell Hall, University of Southampton, Oak Ridge National Laboratory, Max Planck Institute for Extraterrestrial Physics, and Ludwig-Maximilians Universitat Munchen
Subjects: Gravitational Lensing, Cosmology, observations, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cosmology: observations, FOS: Physical sciences, Física, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Dark Energy, Observations [Cosmology], Space and Planetary Science, Weak, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: DES Collaboration: D. Zürcher et al., We constrain the matter density Ωm and the amplitude of density fluctuations σ8 within the ΛCDM cosmological model with shear peak statistics and angular convergence power spectra using mass maps constructed from the first three years of data of the Dark Energy Survey (DES Y3). We use tomographic shear peak statistics, including cross-peaks: peak counts calculated on maps created by taking a harmonic space product of the convergence of two tomographic redshift bins. Our analysis follows a forward-modelling scheme to create a likelihood of these statistics using N-body simulations, using a Gaussian process emulator. We take into account the uncertainty from the remaining, largely unconstrained ΛCDM parameters (Ωb, ns, and h). We include the following lensing systematics: multiplicative shear bias, photometric redshift uncertainty, and galaxy intrinsic alignment. Stringent scale cuts are applied to avoid biases from unmodelled baryonic physics. We find that the additional non-Gaussian information leads to a tightening of the constraints on the structure growth parameter yielding S8 ≡ σ8 √ Ωm/0.3 = 0.797+0.015−0.013 (68 per cent confidence limits), with a precision of 1.8 per cent, an improvement of 38 per cent compared to the angular power spectra only case. The results obtained with the angular power spectra and peak counts are found to be in agreement with each other and no significant difference in S8 is recorded. We find a mild tension of 1.5σ between our study and the results from Planck 2018, with our analysis yielding a lower S8. Furthermore, we observe that the combination of angular power spectra and tomographic peak counts breaks the degeneracy between galaxy intrinsic alignment AIA and S8, improving cosmological constraints. We run a suite of tests concluding that our results are robust and consistent with the results from other studies using DES Y3 data., The ETH Zurich Cosmology group acknowledges support by grants 200021_192243 and 200021_169130 of the Swiss National Science Foundation. We would also like to thank Uwe Schmitt from ETH Zürich for his support with the GitLab server and CI engine. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physic at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnologico and the Ministerio da Ciencia, Tecnologia e Inovacao, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energéticas, Medioambientales y Tecnologicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenoessische Technische Hochschule (ETH) Zurich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciencies de l’Espai (IEEC/CSIC), the Institut de Fisica d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität Muenchen and the associated Excellence Cluster Universe, the University of Michigan, NFS’s NOIRLab, the University of Nottingham, the Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. Based in part on observations at Cerro Tololo Inter-American Observatory at NSF’s NOIRLab (NOIRLab Prop.ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. Based on observations obtained with Planck,11 an ESA science mission with instruments and contributions directly funded by ESA Member States, NASA, and Canada.
Published: 2021

26. Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Data Calibration

Author: Amon, A., Gruen, D., Troxel, M. A., MacCrann, N., Dodelson, S., Choi, A., Doux, C., Secco, L. F., Samuroff, S., Krause, E., Cordero, J., Myles, J., DeRose, J., Wechsler, R. H., Gatti, M., Navarro-Alsina, A., Bernstein, G. M., Jain, B., Blazek, J., Alarcon, A., Ferté, A., Raveri, M., Lemos, P., Campos, A., Prat, J., Sánchez, C., Jarvis, M., Alves, O., Andrade-Oliveira, F., Baxter, E., Bechtol, K., Becker, M. R., Bridle, S. L., Camacho, H., Rosell, A. Carnero, Kind, M. Carrasco, Cawthon, R., Chang, C., Chen, R., Chintalapati, P., Crocce, M., Davis, C., Diehl, H. T., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elvin-Poole, J., Everett, S., Fang, X., Fosalba, P., Friedrich, O., Giannini, G., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Huang, H., Huff, E. M., Huterer, D., Kuropatkin, N., Leget, P. -F., Liddle, A. R., McCullough, J., Muir, J., Pandey, S., Park, Y., Porredon, A., Refregier, A., Rollins, R. P., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Sanchez, J., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troja, A., Tutusaus, I., Varga, T. N., Weaverdyck, N., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Bhargava, S., Brooks, D., Buckley-Geer, E., Burke, D. L., Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Kron, R., Kuehn, K., Lahav, O., Lima, M., Lin, H., Maia, M. A. G., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Petravick, D., Pieres, A., Malagón, A. A. Plazas, Romer, A. K., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Weller, J., Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), DES, Ministerio de Ciencia, Innovación y Universidades (España), Agencia Estatal de Investigación (España), European Commission, European Research Council, Generalitat de Catalunya, Department of Energy (US), National Science Foundation (US), National Aeronautics and Space Administration (US), Ministerio de Economía y Competitividad (España), Amon, A., Gruen, D., Troxel, M. A., Maccrann, N., Dodelson, S., Choi, A., Doux, C., Secco, L. F., Samuroff, S., Krause, E., Cordero, J., Myles, J., Derose, J., Wechsler, R. H., Gatti, M., Navarro-Alsina, A., Bernstein, G. M., Jain, B., Blazek, J., Alarcon, A., Ferte, A., Lemos, P., Raveri, M., Campos, A., Prat, J., Sanchez, C., Jarvis, M., Alves, O., Andrade-Oliveira, F., Baxter, E., Bechtol, K., Becker, M. R., Bridle, S. L., Camacho, H., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Chang, C., Chen, R., Chintalapati, P., Crocce, M., Davis, C., Diehl, H. T., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elvin-Poole, J., Everett, S., Fang, X., Fosalba, P., Friedrich, O., Gaztanaga, E., Giannini, G., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Huang, H., Huff, E. M., Huterer, D., Kuropatkin, N., Leget, P., Liddle, A. R., Mccullough, J., Muir, J., Pandey, S., Park, Y., Porredon, A., Refregier, A., Rollins, R. P., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Sanchez, J., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troja, A., Tutusaus, I., Varga, T. N., Weaverdyck, N., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Bhargava, S., Brooks, D., Buckley-Geer, E., Burke, D. L., Carretero, J., Costanzi, M., Da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., Garcia-Bellido, J., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Kron, R., Kuehn, K., Lahav, O., Lima, M., Lin, H., Maia, M. A. G., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Palmese, A., Paz-Chinchon, F., Petravick, D., Pieres, A., Romer, A. K., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Smith, M., Soares-Santos, M., Tarle, G., Thomas, D., To, C., Weller, J., Stanford University, 382 Via Pueblo Mall, SLAC National Accelerator Laboratory, Duke University, University of Cambridge, Carnegie Mellon University, The Ohio State University, University of Pennsylvania, University of Chicago, University of Arizona, University of Manchester, Lawrence Berkeley National Laboratory, Universidade Estadual de Campinas (UNICAMP), Laboratório Interinstitucional de E-Astronomia, Observatoire de Sauverny, Argonne National Laboratory, California Institute of Technology, University College London, University of Sussex, University of Michigan, Universidade Estadual Paulista (UNESP), University of Wisconsin-Madison, Instituto de Astrofisica de Canarias, Universidad de la Laguna, National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign, Fermi National Accelerator Laboratory, Institut d'Estudis Espacials de Catalunya (IEEC), Institute of Space Sciences (ICE CSIC), Santa Cruz Institute for Particle Physics, The Barcelona Institute of Science and Technology, Denys Wilkinson Building, University of Geneva, University of Edinburgh, Universidade de Lisboa, Perimeter Institute for Theoretical Physics, The University of Tokyo, ETH Zurich, Medioambientales y Tecnológicas (CIEMAT), Brookhaven National Laboratory, Max Planck Institute for Extraterrestrial Physics, Ludwig-Maximilians Universität München, University of Portsmouth, Institut d'Astrophysique de Paris, University of Trieste, INAF-Osservatorio Astronomico di Trieste, Institute for Fundamental Physics of the Universe, Observatório Nacional, IIT Hyderabad, Ludwig-Maximilians-Universität, University of Oslo, Universidad Autonoma de Madrid, University of Queensland, Center for Astrophysics|Harvard and Smithsonian, Macquarie University, Lowell Observatory, Universidade de São Paulo (USP), Texas AandM University, Harvard University, Peyton Hall, Institució Catalana de Recerca i Estudis Avançats, University of Southampton, and UAM. Departamento de Física Teórica
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), microwave background anisotropies, systematic-errors, FOS: Physical sciences, parameter constraints, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, large-scale structure, Astrophysic, weak-lensing surveys, Cosmology and Nongalactic Astrophysics, 0103 physical sciences, internal consistency, Weak, redshift distributions, 010303 astronomy & astrophysics, Gravitational Lensing, 010308 nuclear & particles physics, Física, Dark Energy, intrinsic correlation, matter power spectrum, 2-point correlation-functions, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: DES Collaboration: A. Amon et al., This work, together with its companion paper, Secco, Samuroff et al. [Phys. Rev. D 105, 023515 (2022)], present the Dark Energy Survey Year 3 cosmic-shear measurements and cosmological constraints based on an analysis of over 100 million source galaxies. With the data spanning 4143 deg2 on the sky, divided into four redshift bins, we produce a measurement with a signal-to-noise of 40. We conduct a blind analysis in the context of the Lambda-Cold Dark Matter (ΛCDM) model and find a 3% constraint of the clustering amplitude, S8≡σ8(Ωm/0.3)0.5=0.759+0.025−0.023. A ΛCDM-Optimized analysis, which safely includes smaller scale information, yields a 2% precision measurement of S8=0.772+0.018−0.017 that is consistent with the fiducial case. The two low-redshift measurements are statistically consistent with the Planck Cosmic Microwave Background result, however, both recovered S8 values are lower than the high-redshift prediction by 2.3σ and 2.1σ (p-values of 0.02 and 0.05), respectively. The measurements are shown to be internally consistent across redshift bins, angular scales and correlation functions. The analysis is demonstrated to be robust to calibration systematics, with the S8 posterior consistent when varying the choice of redshift calibration sample, the modeling of redshift uncertainty and methodology. Similarly, we find that the corrections included to account for the blending of galaxies shifts our best-fit S8 by 0.5σ without incurring a substantial increase in uncertainty. We examine the limiting factors for the precision of the cosmological constraints and find observational systematics to be subdominant to the modeling of astrophysics. Specifically, we identify the uncertainties in modeling baryonic effects and intrinsic alignments as the limiting systematics., This research manuscript made use of Astropy [204,205], GetDist [206], ChainConsumer10 [207] and Matplotlib [208], and has been prepared using NASA’s Astrophysics Data System Bibliographic Services. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana- Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministerio da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciencies de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, NFS’s NOIRLab, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. Based in part on observations at Cerro Tololo Inter-American Observatory at NSF’s NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under Grants No. AST-1138766 and No. AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under Grants No. ESP2017-89838, No. PGC2018-094773, No. PGC2018-102021, No. SEV-2016-0588, No. SEV-2016-0597, and No. MDM-2015-0509, some of which include ERDF funds from the European Union. I. F. A. E. is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC Grant agreements No. 240672, No. 291329, and No. 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq Grant No. 465376/2014-2). This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy, Office of Science, and Office of High Energy Physics.
Published: 2021

27. The DECam Local Volume Exploration Survey Data Release 2

Author: Drlica-Wagner, A., Ferguson, P. S., Adamów, M., Aguena, M., Allam, S., Andrade-Oliveira, F., Bacon, D., Bechtol, K., Bell, E. F., Bertin, E., Bilaji, P., Bocquet, S., Bom, C. R., Brooks, D., Burke, D. L., Carballo-Bello, J. A., Carlin, J. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Cerny, W., Chang, C., Choi, Y., Conselice, C., Costanzi, M., Crnojević, D., da Costa, L. N., de Vicente, J., Desai, S., Esteves, J., Everett, S., Ferrero, I., Fitzpatrick, M., Flaugher, B., Friedel, D., Frieman, J., García-Bellido, J., Gatti, M., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Hartley, W. G., Hernandez-Lang, D., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hughes, A. K., Jacques, A., James, D. J., Johnson, M. D., Kuehn, K., Kuropatkin, N., Lahav, O., T. S., Li, Lidman, C., Lin, H., March, M., Marshall, J. L., Martínez-Delgado, D., Martínez-Vázquez, C. E., Massana, P., Mau, S., Mcnanna, M., Melchior, P., Menanteau, F., Miller, A. E., Miquel, R., Mohr, J. J., Morgan, R., Mutlu-Pakdil, B., Muñoz, R. R., Neilsen, E. H., Nidever, D. L., Nikutta, R., Nilo Castellon, J. L., Noël, N. E. D., Ogando, R. L. C., Olsen, K. A. G., Pace, A. B., Palmese, A., Paz-Chinchón, F., Pereira, M. E. S., Pieres, A., Plazas Malagón, A. A., Prat, J., Riley, A. H., Rodriguez-Monroy, M., Romer, A. K., Roodman, A., Sako, M., Sakowska, J. D., Sanchez, E., Sánchez, F. J., Sand, D. J., Santana-Silva, L., Santiago, B., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Simon, J. D., Smith, M., Soares-Santos, M., Stringfellow, G. S., Suchyta, E., Suson, D. J., Tan, C. Y., Tarle, G., Tavangar, K., Thomas, D., To, C., Tollerud, E. J., Troxel, M. A., Tucker, D. L., Varga, T. N., Vivas, A. K., Walker, A. R., Weller, J., Wilkinson, R. D., J. F., Wu, Yanny, B., Zaborowski, E., Zenteno, A., Delve, Collaboration, Des, Collaboration, Astro Data Lab, Drlica-Wagner, A., Ferguson, P. S., Adamów, M., Aguena, M., Allam, S., Andrade-Oliveira, F., Bacon, D., Bechtol, K., Bell, E. F., Bertin, E., Bilaji, P., Bocquet, S., Bom, C. R., Brooks, D., Burke, D. L., Carballo-Bello, J. A., Carlin, J. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Cerny, W., Chang, C., Choi, Y., Conselice, C., Costanzi, M., Crnojević, D., da Costa, L. N., de Vicente, J., Desai, S., Esteves, J., Everett, S., Ferrero, I., Fitzpatrick, M., Flaugher, B., Friedel, D., Frieman, J., García-Bellido, J., Gatti, M., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Hartley, W. G., Hernandez-Lang, D., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hughes, A. K., Jacques, A., James, D. J., Johnson, M. D., Kuehn, K., Kuropatkin, N., Lahav, O., T. S., Li, Lidman, C., Lin, H., March, M., Marshall, J. L., Martínez-Delgado, D., Martínez-Vázquez, C. E., Massana, P., Mau, S., Mcnanna, M., Melchior, P., Menanteau, F., Miller, A. E., Miquel, R., Mohr, J. J., Morgan, R., Mutlu-Pakdil, B., Muñoz, R. R., Neilsen, E. H., Nidever, D. L., Nikutta, R., Nilo Castellon, J. L., Noël, N. E. D., Ogando, R. L. C., Olsen, K. A. G., Pace, A. B., Palmese, A., Paz-Chinchón, F., Pereira, M. E. S., Pieres, A., Plazas Malagón, A. A., Prat, J., Riley, A. H., Rodriguez-Monroy, M., Romer, A. K., Roodman, A., Sako, M., Sakowska, J. D., Sanchez, E., Sánchez, F. J., Sand, D. J., Santana-Silva, L., Santiago, B., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Simon, J. D., Smith, M., Soares-Santos, M., Stringfellow, G. S., Suchyta, E., Suson, D. J., Tan, C. Y., Tarle, G., Tavangar, K., Thomas, D., To, C., Tollerud, E. J., Troxel, M. A., Tucker, D. L., Varga, T. N., Vivas, A. K., Walker, A. R., Weller, J., Wilkinson, R. D., J. F., Wu, Yanny, B., Zaborowski, E., Zenteno, A., Delve, Collaboration, Des, Collaboration, Astro Data Lab, Ministerio de Ciencia e Innovación (España), European Commission, European Research Council, and Fundação de Amparo à Pesquisa do Estado de São Paulo
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Astronomy and Astrophysics, Surveys, Astrophysics - Astrophysics of Galaxies, Catalogs, Local Group, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Catalog, Survey, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Full list of authors: Drlica-Wagner, A.; Ferguson, P. S.; Adamow, M.; Aguena, M.; Allam, S.; Andrade-Oliveira, F.; Bacon, D.; Bechtol, K.; Bell, E. F.; Bertin, E.; Bilaji, P.; Bocquet, S.; Bom, C. R.; Brooks, D.; Burke, D. L.; Carballo-Bello, J. A.; Carlin, J. L.; Carnero Rosell, A.; Kind, M. Carrasco; Carretero, J.; Castander, F. J.; Cerny, W.; Chang, C.; Choi, Y.; Conselice, C.; Costanzi, M.; Crnojevic, D.; da Costa, L. N.; De Vicente, J.; Desai, S.; Esteves, J.; Everett, S.; Ferrero, I; Fitzpatrick, M.; Flaugher, B.; Friedel, D.; Frieman, J.; Garcia-Bellido, J.; Gatti, M.; Gaztanaga, E.; Gerdes, D. W.; Gruen, D.; Gruendl, R. A.; Gschwend, J.; Hartley, W. G.; Hernandez-Lang, D.; Hinton, S. R.; Hollowood, D. L.; Honscheid, K.; Hughes, A. K.; Jacques, A.; James, D. J.; Johnson, M. D.; Kuehn, K.; Kuropatkin, N.; Lahav, O.; Li, T. S.; Lidman, C.; Lin, H.; March, M.; Marshall, J. L.; Martinez-Delgado, D.; Martinez-Vazquez, C. E.; Massana, P.; Mau, S.; McNanna, M.; Melchior, P.; Menanteau, F.; Miller, A. E.; Miquel, R.; Mohr, J. J.; Morgan, R.; Mutlu-Pakdil, B.; Munoz, R. R.; Neilsen, E. H.; Nidever, D. L.; Nikutta, R.; Nilo Castellon, J. L.; Noel, N. E. D.; Ogando, R. L. C.; Olsen, K. A. G.; Pace, A. B.; Palmese, A.; Paz-Chinchon, F.; Pereira, M. E. S.; Pieres, A.; Malagon, A. A. Plazas; Prat, J.; Riley, A. H.; Rodriguez-Monroy, M.; Romer, A. K.; Roodman, A.; Sako, M.; Sakowska, J. D.; Sanchez, E.; Sanchez, F. J.; Sand, D. J.; Santana-Silva, L.; Santiago, B.; Schubnell, M.; Serrano, S.; Sevilla-Noarbe, I; Simon, J. D.; Smith, M.; Soares-Santos, M.; Stringfellow, G. S.; Suchyta, E.; Suson, D. J.; Tan, C. Y.; Tarle, G.; Tavangar, K.; Thomas, D.; To, C.; Tollerud, E. J.; Troxel, M. A.; Tucker, D. L.; Varga, T. N.; Vivas, A. K.; Walker, A. R.; Weller, J.; Wilkinson, R. D.; Wu, J. F.; Yanny, B.; Zaborowski, E.; Zenteno, A.; DELVE Collaboration; DES Collaboration; Astro Data Lab.--This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited., We present the second public data release (DR2) from the DECam Local Volume Exploration survey (DELVE). DELVE DR2 combines new DECam observations with archival DECam data from the Dark Energy Survey, the DECam Legacy Survey, and other DECam community programs. DELVE DR2 consists of ∼160,000 exposures that cover >21,000 deg2 of the high-Galactic-latitude (∣b∣ > 10°) sky in four broadband optical/near-infrared filters (g, r, i, z). DELVE DR2 provides point-source and automatic aperture photometry for ∼2.5 billion astronomical sources with a median 5σ point-source depth of g = 24.3, r = 23.9, i = 23.5, and z = 22.8 mag. A region of ∼17,000 deg2 has been imaged in all four filters, providing four-band photometric measurements for ∼618 million astronomical sources. DELVE DR2 covers more than 4 times the area of the previous DELVE data release and contains roughly 5 times as many astronomical objects. DELVE DR2 is publicly available via the NOIRLab Astro Data Lab science platform. © 2022. The Author(s). Published by the American Astronomical Society., The DELVE project is partially supported by Fermilab LDRD project L2019-011, the NASA Fermi Guest Investigator Program Cycle 9 grant 91201, and the National Science Foundation (NSF) under grant AST-2108168. This work is supported by the Fermilab Visiting Scholars Award Program from the Universities Research Association. A.B.P. acknowledges support from NSF grant AST-1813881. J.L.C. acknowledges support from NSF grant AST-1816196. J.D.S. acknowledges support from NSF grant AST-1714873. S.R.M. acknowledges support from NSF grant AST-1909497. D.J.S. acknowledges support from NSF grants AST-1821967 and AST-1813708. D.C. acknowledges support from NSF grant AST-1814208. B.M.P. acknowledges support from the NSF Astronomy and Astrophysics Postdoctoral Fellowship under award AST-2001663. S.M. acknowledges support from the NSF Graduate Research Fellowship under grant DGE-1656518. D.M.D. acknowledges financial support from the State Agency for Research of the Spanish MCIU through the "Centre of Excellence Severo Ochoa" award for the Instituto de Astrofísica de Andalucía (SEV-2017-0709). C.P.M.B. and M.R.L.C. acknowledge support from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (grant agreement no. 682115). L.S.S. acknowledges the financial support from FAPESP through the grant #2020/03301-5. J.A.C.B. acknowledges support from ANID FONDECYT Regular 1220083. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo á Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciències de l'Espai (IEEC/CSIC), the Institut de Física d'Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, NSF's NOIRLab, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. The DES data management system is supported by the National Science Foundation under grant Nos. AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under grants ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Program (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq grant 465376/2014-2).
Published: 2022

28. Present clinical practice of breast cancer radiotherapy in Italy: a nationwide survey by the Italian Society of Radiotherapy and Clinical Oncology (AIRO) Breast Group

Author: Gregucci, F., Fozza, A., Falivene, S., Smaniotto, D., Morra, A., Daidone, A., Barbara, R., Ciabattoni, A., Andrulli, D., Arcidiacono, F., Baiocchi, C., Baldissera, A., Barbarino, R., Bartoncini, S., Bono, M., Buffoli, A., Campanella, B., Campoccia, S., Catalano, G., Cavallari, M., Cerreta, V., Deantonio, L., De Rose, F., Del Bufalo, S., Digennaro, D., Doino, D., Evangelista, G., Fedele, F., Fiorentino, A., Fodor, A., Fontana, A., Fusco, V., Gatti, M., Gerardi, M., Giannini, M., Girlando, A., Guenzi, M., Guida, C., Huscher, A., Iannone, T., Iorio, V., Ippolito, E., Ivaldi, G., La Porta, M., Lazzari, G., Lioce, M., Lora, O., Macchia, G., Mangiacotti, M. G., Marafioti, L., Marino, L., Marmiroli, L., Maucieri, A., Maurizi, F., Mazzuoli, L., Meattini, I., Meduri, B., Montesi, G., Munoz, F., Nuzzo, M., Orru, S., Parisi, S., Pasinetti, N., Pedretti, S., Perrucci, E., Piva, D., Prisco, A., Ravo, V., Santacaterina, A., Scolaro, T., Serafini, F., Spigone, B., Tolento, G., Vidali, C., Vitucci, P., and Zini, G.
Subjects: Hypofractionated Radiotherapy, medicine.medical_specialty, medicine.medical_treatment, Breast Neoplasms, Breast cancer radiotherapy, Nationwide survey, Hypofractionated radiotherapy, 030218 nuclear medicine & medical imaging, AIRO, Breast cancer, Partial-breast irradiation, Radiotherapy and neoadjuvant therapy, Re-irradiation, Survey, 03 medical and health sciences, 0302 clinical medicine, Surveys and Questionnaires, medicine, Humans, Radiology, Nuclear Medicine and imaging, Practice Patterns, Physicians', Medical prescription, Societies, Medical, Clinical Oncology, business.industry, General surgery, Radiation Oncologists, General Medicine, medicine.disease, Clinical Practice, Radiation therapy, Italy, 030220 oncology & carcinogenesis, Female, business
Abstract: To investigate the present attitude of the Italian Radiation Oncologists in the management of breast cancer (BC) concerning hypofractionated radiotherapy (hRT), partial-breast irradiation (PBI), re-irradiation (rRT) and radiotherapy after neoadjuvant chemotherapy (post-NAC RT). A nationwide, 21-point questionnaire was distributed online via SurveyMonkey. Seventy-four Italian Radiotherapy Centers answered to the survey. In most cases, the responding centers treated more than 100 BC patients/year between January 2016 and December 2017. Almost half of responding centers (49%) treated patients with hRT, out of these, 95% as routine practice for early-stage BC. Dose prescriptions ranged between 39 and 45 Gy indicating a high use of moderate hRT. The chest wall and regional lymph nodes were irradiated with hRT by 13% and 15% of the responding centers, respectively. PBI was used by 60% of responders, with different techniques. Only 0.6% of participants perform rRT after BC recurrence. Finally, only 11% of the interviewed centers responded to their attitude toward post-NAC RT, which, however, was indicated in 97% of patients after breast-conserving surgery. This survey shows a fairly good use of hRT and a moderate practice of PBI in Italy. Some practices like hRT to the chest wall and regional lymph nodes as well as rRT need further verification. Likewise, the management of post-NAC RT is very heterogeneous. Future national clinical collaborative studies are advocated in order to investigate these controversial topics about breast cancer radiotherapy.
Published: 2020

29. Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing

Author: Abbott, TMC, Aguena, M, Alarcon, A, Allam, S, Alves, O, Amon, A, Andrade-Oliveira, F, Annis, J, Avila, S, Bacon, D, Baxter, E, Bechtol, K, Becker, MR, Bernstein, GM, Bhargava, S, Birrer, S, Blazek, J, Brandao-Souza, A, Bridle, SL, Brooks, D, Buckley-Geer, E, Burke, DL, Camacho, H, Campos, A, Rosell, A Carnero, Kind, M Carrasco, Carretero, J, Castander, FJ, Cawthon, R, Chang, C, Chen, A, Chen, R, Choi, A, Conselice, C, Cordero, J, Costanzi, M, Crocce, M, da Costa, LN, da Silva Pereira, ME, Davis, C, Davis, TM, De Vicente, J, DeRose, J, Desai, S, Di Valentino, E, Diehl, HT, Dietrich, JP, Dodelson, S, Doel, P, Doux, C, Drlica-Wagner, A, Eckert, K, Eifler, TF, Elsner, F, Elvin-Poole, J, Everett, S, Evrard, AE, Fang, X, Farahi, A, Fernandez, E, Ferrero, I, Ferté, A, Fosalba, P, Friedrich, O, Frieman, J, García-Bellido, J, Gatti, M, Gaztanaga, E, Gerdes, DW, Giannantonio, T, Giannini, G, Gruen, D, Gruendl, RA, Gschwend, J, Gutierrez, G, Harrison, I, Hartley, WG, Herner, K, Hinton, SR, Hollowood, DL, Honscheid, K, Hoyle, B, Huff, EM, Huterer, D, Jain, B, James, DJ, Jarvis, M, Jeffrey, N, Jeltema, T, Kovacs, A, Krause, E, Kron, R, Kuehn, K, Kuropatkin, N, Lahav, O, Leget, P-F, Lemos, P, Liddle, AR, Lidman, C, and Lima, M
Subjects: Quantum Physics, Particle and Plasma Physics, Molecular, Nuclear, Atomic, Nuclear & Particles Physics, Astronomical and Space Sciences
Abstract: We present the first cosmology results from large-scale structure using the full 5000 deg2 of imaging data from the Dark Energy Survey (DES) Data Release 1. We perform an analysis of large-scale structure combining three two-point correlation functions (3×2pt): (i) cosmic shear using 100 million source galaxies, (ii) galaxy clustering, and (iii) the cross-correlation of source galaxy shear with lens galaxy positions, galaxy-galaxy lensing. To achieve the cosmological precision enabled by these measurements has required updates to nearly every part of the analysis from DES Year 1, including the use of two independent galaxy clustering samples, modeling advances, and several novel improvements in the calibration of gravitational shear and photometric redshift inference. The analysis was performed under strict conditions to mitigate confirmation or observer bias; we describe specific changes made to the lens galaxy sample following unblinding of the results and tests of the robustness of our results to this decision. We model the data within the flat ΛCDM and wCDM cosmological models, marginalizing over 25 nuisance parameters. We find consistent cosmological results between the three two-point correlation functions; their combination yields clustering amplitude S8=0.776-0.017+0.017 and matter density ωm=0.339-0.031+0.032 in ΛCDM, mean with 68% confidence limits; S8=0.775-0.024+0.026, ωm=0.352-0.041+0.035, and dark energy equation-of-state parameter w=-0.98-0.20+0.32 in wCDM. These constraints correspond to an improvement in signal-to-noise of the DES Year 3 3×2pt data relative to DES Year 1 by a factor of 2.1, about 20% more than expected from the increase in observing area alone. This combination of DES data is consistent with the prediction of the model favored by the Planck 2018 cosmic microwave background (CMB) primary anisotropy data, which is quantified with a probability-to-exceed p=0.13-0.48. We find better agreement between DES 3×2pt and Planck than in DES Y1, despite the significantly improved precision of both. When combining DES 3×2pt data with available baryon acoustic oscillation, redshift-space distortion, and type Ia supernovae data, we find p=0.34. Combining all of these datasets with Planck CMB lensing yields joint parameter constraints of S8=0.812-0.008+0.008, ωm=0.306-0.005+0.004, h=0.680-0.003+0.004, and mν
Published: 2022

30. Photometric Properties of Jupiter Trojans detected by the Dark Energy Survey

Author: Collobration, DES, Pan, Jiaming, Lin, Hsing Wen, Gerdes, David W., Napier, Kevin J., Wang, Jichi, Abbott, T. M. C., Aguena, M., Allam, S., Alves, O., Bacon, D., Bernardinelli, P. H., Bernstein, G. M., Bertin, E., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Doel, P., Ferrero, I., Friedel, D., Frieman, J., García-Bellido, J., Gatti, M., Gruendl, R. A., Gschwend, J., Herner, K., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Kuropatkin, N., March, M., Menanteau, F., Miquel, R., Paz-Chinchón, F., Pieres, A., Malagón, A. A. Plazas, Raveri, M., Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Tarle, G., Tucker, D., Walker, A. R., and Weaverdyck, N.
Subjects: Earth and Planetary Astrophysics (astro-ph.EP), FOS: Physical sciences, Astrophysics - Earth and Planetary Astrophysics
Abstract: The Jupiter Trojans are a large group of asteroids that are co-orbiting with Jupiter near its L4 and L5 Lagrange points. The study of Jupiter Trojans is crucial for testing different models of planet formation that are directly related to our understanding of solar system evolution. In this work, we select known Jupiter Trojans listed by the Minor Planet Center (MPC) from the full six years dataset (Y6) of the Dark Energy Survey (DES) to analyze their photometric properties. The DES data allow us to study Jupiter Trojans with a fainter magnitude limit than previous studies in a homogeneous survey with $griz$ band measurements. We extract a final catalog of 573 unique Jupiter Trojans. Our sample include 547 asteroids belonging to L5. This is one of the largest analyzed samples for this group. By comparing with the data reported by other surveys we found that the color distribution of L5 Trojans is similar to that of L4 Trojans. We find that L5 Trojans' $g - i$ and $g - r$ colors become less red with fainter absolute magnitudes, a trend also seen in L4 Trojans. Both the L4 and L5 clouds consistently show such a color-size correlation over an absolute magnitude range $11 < H < 18$. We also use DES colors to perform taxonomic classifications. C and P-type asteroids outnumber D-type asteroids in the L5 Trojans DES sample, which have diameters in the 5 - 20 km range. This is consistent with the color-size correlation., This manuscript is accepted for publication in PSJ. There is a full version of table 1
Published: 2022
Full Text: View/download PDF

31. Dark Energy Survey Year 3 Results: Three-Point Shear Correlations and Mass Aperture Moments

Author: Secco, Lucas F., Jarvis, M., Jain, B., Chang, C., Gatti, M., Frieman, J., Adhikari, S., Alarcon, A., Amon, A., Bechtol, K., Becker, M.R., Bernstein, G.M., Blazek, J., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Choi, A., Cordero, J., DeRose, J., Dodelson, S., Doux, C., Drlica-Wagner, A., Everett, S., Giannini, G., Gruen, D., Gruendl, R.A., Harrison, I., Hartley, W.G., Herner, K., Krause, E., MacCrann, N., McCullough, J., Myles, J., Navarro-Alsina, A., Prat, J., Rollins, R.P., Samuroff, S., Sánchez, C., Sevilla-Noarbe, I., Sheldon, E., Troxel, M.A., Zeurcher, D., Aguena, M., Andrade-Oliveira, F., Annis, J., Bacon, D., Bertin, E., Bocquet, S., Brooks, D., Burke, D.L., Carretero, J., Castander, F.J., Crocce, M., da Costa, L.N., Pereira, M.E.S., De Vicente, J., Diehl, H.T., Doel, P., Eckert, K., Ferrero, Ismael, Flaugher, B., Friedel, D., García-Bellido, J., Gutierrez, G., Hinton, S.R., Hollowood, D.L., Honscheid, K., Huterer, D., Kuehn, K., Kuropatkin, N., Maia, M.A.G., Marshall, J.L., Menanteau, F., Miquel, R., Mohr, J.J., Morgan, R., Muir, J., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A.A., Rodriguez-Monroy, M., Roodman, A., Sanchez, E., Serrano, S., Suchyta, E., Swanson, M.E.C., Tarle, G., Thomas, D., To, C., Weller, J., National Science Foundation (US), Department of Energy (US), Ministerio de Educación y Ciencia (España), Agencia Estatal de Investigación (España), Science and Technology Facilities Council (UK), Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), European Research Council, European Commission, Generalitat de Catalunya, and UAM. Departamento de Física Teórica
Subjects: Gravitational Lensing, Quantum Physics, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Física, Molecular, FOS: Physical sciences, prospects, Astrophysics::Cosmology and Extragalactic Astrophysics, calibration, Dark Energy, Atomic, Nuclear & Particles Physics, weak-lensing surveys, Particle and Plasma Physics, cosmological constraints, cfhtlens, model predictions, Nuclear, Weak, higher-order statistics, cosmic shear, Astronomical and Space Sciences, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: DES Collaboration: L. F. Secco et al., We present high signal-to-noise measurements of three-point shear correlations and the third moment of the mass aperture statistic using the first 3 years of data from the Dark Energy Survey. We additionally obtain the first measurements of the configuration and scale dependence of the four three-point shear correlations which carry cosmological information. With the third-order mass aperture statistic, we present tomographic measurements over angular scales of 4 to 60 arcminutes with a combined statistical significance of 15.0σ. Using the tomographic information and measuring also the second-order mass aperture, we additionally obtain a skewness parameter and its redshift evolution. We find that the amplitudes and scale-dependence of these shear 3pt functions are in qualitative agreement with measurements in a mock galaxy catalog based on N-body simulations, indicating promise for including them in future cosmological analyses. We validate our measurements by showing that B-modes, parity-violating contributions and PSF modeling uncertainties are negligible, and determine that the measured signals are likely to be of astrophysical and gravitational origin., M. J. is supported in part by National Science Foundation Grant No. 1907610. B. J. is supported in part by the U.S. Department of Energy Grant No. DE-SC0007901. C. C. is supported by DOE grant DE-SC0021949. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministerio da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciencies de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. The DES data management system is supported by the National Science Foundation under Grants No. AST-1138766 and No. AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under Grants No. ESP2017-89838, No. PGC2018-094773, No. PGC2018-102021, No. SEV-2016-0588, No. SEV-2016-0597, and No. MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC Grants agreements No. 240672, No. 291329, and No. 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) do e-Universo (CNPq Grant No. 465376/2014-2). We acknowledge support from the Australian Research Council Centre of Excellence for Allsky Astrophysics (CAASTRO), through Project No. CE110001020. This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DEAC02-07CH11359 with the U.S. Department of Energy, Office of Science, Office of High Energy Physics.
Published: 2022
Full Text: View/download PDF

32. The DECam Local Volume Exploration Survey Data Release 2

Author: Drlica-Wagner, A, Ferguson, PS, Adamów, M, Aguena, M, Allam, S, Andrade-Oliveira, F, Bacon, D, Bechtol, K, Bell, EF, Bertin, E, Bilaji, P, Bocquet, S, Bom, CR, Brooks, D, Burke, DL, Carballo-Bello, JA, Carlin, JL, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Castander, FJ, Cerny, W, Chang, C, Choi, Y, Conselice, C, Costanzi, M, Crnojević, D, Da Costa, LN, De Vicente, J, Desai, S, Esteves, J, Everett, S, Ferrero, I, Fitzpatrick, M, Flaugher, B, Friedel, D, Frieman, J, García-Bellido, J, Gatti, M, Gaztanaga, E, Gerdes, DW, Gruen, D, Gruendl, RA, Gschwend, J, Hartley, WG, Hernandez-Lang, D, Hinton, Hollowood, DL, Honscheid, K, Hughes, AK, Jacques, A, James, DJ, Johnson, MD, Kuehn, K, Kuropatkin, N, Lahav, O, Li, TS, Lidman, C, Lin, H, March, M, Marshall, JL, Martínez-Delgado, D, Martínez-Vázquez, CE, Massana, P, Mau, S, McNanna, M, Melchior, P, Menanteau, F, Miller, AE, Miquel, R, Mohr, JJ, Morgan, R, Mutlu-Pakdil, B, Muñoz, RR, Neilsen, EH, Nidever, DL, Nikutta, R, Nilo Castellon, JL, Noël, NED, Ogando, RLC, Olsen, KAG, Pace, AB, Palmese, A, Paz-Chinchón, F, Pereira, MES, Pieres, A, Plazas Malagón, AA, Prat, J, Riley, AH, Rodriguez-Monroy, M, Romer, AK, Roodman, A, Sako, M, Sakowska, JD, Sanchez, E, Sánchez, FJ, Sand, DJ, Santana-Silva, L, Santiago, B, Schubnell, M, Drlica-Wagner, A [0000-0001-8251-933X], Ferguson, PS [0000-0001-6957-1627], Adamów, M [0000-0002-6904-359X], Aguena, M [0000-0001-5679-6747], Bacon, D [0000-0002-2562-8537], Bechtol, K [0000-0001-8156-0429], Bell, EF [0000-0002-5564-9873], Bertin, E [0000-0002-3602-3664], Bocquet, S [0000-0002-4900-805X], Bom, CR [0000-0003-4383-2969], Brooks, D [0000-0002-8458-5047], Carballo-Bello, JA [0000-0002-3690-105X], Carlin, JL [0000-0002-3936-9628], Carnero Rosell, A [0000-0003-3044-5150], Carrasco Kind, M [0000-0002-4802-3194], Carretero, J [0000-0002-3130-0204], Castander, FJ [0000-0001-7316-4573], Cerny, W [0000-0003-1697-7062], Chang, C [0000-0002-7887-0896], Conselice, C [0000-0003-1949-7638], Costanzi, M [0000-0001-8158-1449], Crnojević, D [0000-0002-1763-4128], De Vicente, J [0000-0001-8318-6813], Desai, S [0000-0002-0466-3288], Fitzpatrick, M [0000-0002-9080-0751], Flaugher, B [0000-0002-2367-5049], Frieman, J [0000-0003-4079-3263], García-Bellido, J [0000-0002-9370-8360], Gaztanaga, E [0000-0001-9632-0815], Gerdes, DW [0000-0001-6942-2736], Gruen, D [0000-0003-3270-7644], Gruendl, RA [0000-0002-4588-6517], Gschwend, J [0000-0003-3023-8362], Hinton, SR [0000-0003-2071-9349], Hollowood, DL [0000-0002-9369-4157], Honscheid, K [0000-0002-6550-2023], Hughes, AK [0000-0002-1718-0402], Jacques, A [0000-0001-9631-831X], James, DJ [0000-0001-5160-4486], Kuehn, K [0000-0003-0120-0808], Kuropatkin, N [0000-0003-2511-0946], Lahav, O [0000-0002-1134-9035], Li, TS [0000-0002-9110-6163], Lidman, C [0000-0003-1731-0497], Lin, H [0000-0002-7825-3206], Marshall, JL [0000-0003-0710-9474], Martínez-Delgado, D [0000-0003-3835-2231], Martínez-Vázquez, CE [0000-0002-9144-7726], Massana, P [0000-0002-8093-7471], Mau, S [0000-0003-3519-4004], McNanna, M [0000-0001-5435-7820], Melchior, P [0000-0002-8873-5065], Menanteau, F [0000-0002-1372-2534], Miller, AE [0000-0002-7483-7327], Miquel, R [0000-0002-6610-4836], Mohr, JJ [0000-0002-0810-5558], Morgan, R [0000-0002-7016-5471], Mutlu-Pakdil, B [0000-0001-9649-4815], Neilsen, EH [0000-0002-7357-0317], Nidever, DL [0000-0002-1793-3689], Nikutta, R [0000-0002-7052-6900], Nilo Castellon, JL [0000-0002-8282-469X], Ogando, RLC [0000-0003-2120-1154], Olsen, KAG [0000-0002-7134-8296], Pace, AB [0000-0002-6021-8760], Palmese, A [0000-0002-6011-0530], Paz-Chinchón, F [0000-0003-1339-2683], Pieres, A [0000-0001-9186-6042], Plazas Malagón, AA [0000-0002-2598-0514], Riley, AH [0000-0001-5805-5766], Romer, AK [0000-0002-9328-879X], Roodman, A [0000-0001-5326-3486], Sako, M [0000-0003-2764-7093], Sakowska, JD [0000-0002-1594-1466], Sanchez, E [0000-0002-9646-8198], Sánchez, FJ [0000-0003-3136-9532], Sand, DJ [0000-0003-4102-380X], Santana-Silva, L [0000-0003-3402-6164], Schubnell, M [0000-0001-9504-2059], and Apollo - University of Cambridge Repository
Subjects: astro-ph.GA, astro-ph.CO, astro-ph.IM
Abstract: We present the second public data release (DR2) from the DECam Local Volume Exploration survey (DELVE). DELVE DR2 combines new DECam observations with archival DECam data from the Dark Energy Survey, the DECam Legacy Survey, and other DECam community programs. DELVE DR2 consists of ~160,000 exposures that cover >21,000 deg^2 of the high Galactic latitude (|b| > 10 deg) sky in four broadband optical/near-infrared filters (g, r, i, z). DELVE DR2 provides point-source and automatic aperture photometry for ~2.5 billion astronomical sources with a median 5{\sigma} point-source depth of g=24.3, r=23.9, i=23.5, and z=22.8 mag. A region of ~17,000 deg^2 has been imaged in all four filters, providing four-band photometric measurements for ~618 million astronomical sources. DELVE DR2 covers more than four times the area of the previous DELVE data release and contains roughly five times as many astronomical objects. DELVE DR2 is publicly available via the NOIRLab Astro Data Lab science platform.
Published: 2022

33. Joint analysis of DES Year 3 data and CMB lensing from SPT and Planck I: Construction of CMB Lensing Maps and Modeling Choices

Author: Omori, Y., Baxter, E. J., Chang, C., Friedrich, O., Alarcon, A., Alves, O., Amon, A., Andrade-Oliveira, F., Bechtol, K., Becker, M. R., Bernstein, G. M., Blazek, J., Bleem, L. E., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Chen, R., Choi, A., Cordero, J., Crawford, T. M., Crocce, M., Davis, C., Derose, J., Dodelson, S., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Elvin-Poole, J., Everett, S., Fang, X., Ferté, A., Fosalba, P., Gatti, M., Giannini, G., Gruen, D., Gruendl, R. A., Harrison, I., Herner, K., Huang, H., Huff, E. M., Huterer, D., Jarvis, M., Krause, E., Kuropatkin, N., Leget, P. -F, Pablo Lemos, Liddle, A. R., Maccrann, N., Mccullough, J., Muir, J., Myles, J., Navarro-Alsina, A., Pandey, S., Park, Y., Porredon, A., Prat, J., Raveri, M., Rollins, R. P., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Sánchez, C., Sanchez, J., Secco, L. F., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troxel, M. A., Tutusaus, I., Varga, T. N., Weaverdyck, N., Wechsler, R. H., Wu, W. L. K., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Bacon, D., Benson, B. A., Bertin, E., Bocquet, S., Brooks, D., Burke, D. L., Carlstrom, J. E., Carretero, J., Chang, C. L., Chown, R., Costanzi, M., Da Costa, L. N., Crites, A. T., Pereira, M. E. S., Haan, T., Vicente, J., Desai, S., Diehl, H. T., Dobbs, M. A., Doel, P., Everett, W., Ferrero, I., Flaugher, B., Friedel, D., Frieman, J., García-Bellido, J., Gaztanaga, E., George, E. M., Giannantonio, T., Halverson, N. W., Hinton, S. R., Holder, G. P., Hollowood, D. L., Holzapfel, W. L., Honscheid, K., Hrubes, J. D., James, D. J., Knox, L., Kuehn, K., Lahav, O., Lee, A. T., Lima, M., Luong-Van, D., March, M., Mcmahon, J. J., Melchior, P., Menanteau, F., Meyer, S. S., Miquel, R., Mocanu, L., Mohr, J. J., Morgan, R., Natoli, T., Padin, S., Palmese, A., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A. A., Pryke, C., Reichardt, C. L., Romer, A. K., Ruhl, J. E., Sanchez, E., Schaffer, K. K., Schubnell, M., Serrano, S., Shirokoff, E., Smith, M., Staniszewski, Z., Stark, A. A., Suchyta, E., Tarle, G., Thomas, D., To, C., Vieira, J. D., Weller, J., and Williamson, R.
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Joint analyses of cross-correlations between measurements of galaxy positions, galaxy lensing, and lensing of the cosmic microwave background (CMB) offer powerful constraints on the large-scale structure of the Universe. In a forthcoming analysis, we will present cosmological constraints from the analysis of such cross-correlations measured using Year 3 data from the Dark Energy Survey (DES), and CMB data from the South Pole Telescope (SPT) and Planck. Here we present two key ingredients of this analysis: (1) an improved CMB lensing map in the SPT-SZ survey footprint, and (2) the analysis methodology that will be used to extract cosmological information from the cross-correlation measurements. Relative to previous lensing maps made from the same CMB observations, we have implemented techniques to remove contamination from the thermal Sunyaev Zel'dovich effect, enabling the extraction of cosmological information from smaller angular scales of the cross-correlation measurements than in previous analyses with DES Year 1 data. We describe our model for the cross-correlations between these maps and DES data, and validate our modeling choices to demonstrate the robustness of our analysis. We then forecast the expected cosmological constraints from the galaxy survey-CMB lensing auto and cross-correlations. We find that the galaxy-CMB lensing and galaxy shear-CMB lensing correlations will on their own provide a constraint on $S_8=\sigma_8 \sqrt{\Omega_{\rm m}/0.3}$ at the few percent level, providing a powerful consistency check for the DES-only constraints. We explore scenarios where external priors on shear calibration are removed, finding that the joint analysis of CMB lensing cross-correlations can provide constraints on the shear calibration amplitude at the 5 to 10% level., Comment: 30 pages, 20 figures, To be submitted to PRD
Published: 2022
Full Text: View/download PDF

34. A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES

Author: Schiappucci, E., Bianchini, F., Aguena, M., Archipley, M., Balkenhol, L., Bleem, L. E., Chaubal, P., Crawford, T. M., Grandis, S., Omori, Y., Reichardt, C. L., Rozo, E., Rykoff, E. S., To, C., Abbott, T. M. C., Ade, P. A. R., Alves, O., Anderson, A. J., Andrade-Oliveira, F., Annis, J., Avva, J. S., Bacon, D., Benabed, K., Bender, A. N., Benson, B. A., Bernstein, G. M., Bertin, E., Bocquet, S., Bouchet, F. R., Brooks, D., Burke, D. L., Carlstrom, J. E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cecil, T. W., Chang, C. L., Chichura, P. M., Chou, T. -L., Costanzi, M., Cukierman, A., da Costa, L. N., Daley, C., de Haan, T., Desai, S., Dibert, K. R., Diehl, H. T., Dobbs, M. A., Doel, P., Doux, C., Dutcher, D., Everett, S., Everett, W., Feng, C., Ferguson, K. R., Ferrero, I., Ferté, A., Flaugher, B., Foster, A., Frieman, J., Galli, S., Gambrel, A. E., García-Bellido, J., Gardner, R. W., Gatti, M., Giannantonio, T., Goeckner-Wald, N., Gruen, D., Gualtieri, R., Guns, S., Gutierrez, G., Halverson, N. W., Hinton, S. R., Hivon, E., Holder, G. P., Hollowood, D. L., Holzapfel, W. L., Honscheid, K., Hood, J. C., Huang, N., James, D. J., Knox, L., Korman, M., Kuehn, K., Kuo, C. -L., Lahav, O., Lee, A. T., Lidman, C., Lima, M., Lowitz, A. E., Lu, C., March, M., Mena-Fernández, J., Menanteau, F., Millea, M., Miquel, R., Mohr, J. J., Montgomery, J., Muir, J., Natoli, T., Noble, G. I., Novosad, V., Ogando, R. L. C., Padin, S., Pan, Z., Paz-Chinchón, F., Pereira, M. E. S., Pieres, A., Malagón, A. A. Plazas, Prabhu, K., Prat, J., Quan, W., Rahlin, A., Raveri, M., Rodriguez-Monroy, M., Romer, A. K., Rouble, M., Ruhl, J. E., Sanchez, E., Scarpine, V., Schubnell, M., Smecher, G., Smith, M., Soares-Santos, M., Sobrin, J. A., Suchyta, E., Suzuki, A., Tarle, G., Thomas, D., Thompson, K. L., Thorne, B., Tucker, C., Umilta, C., Vieira, J. D., Vincenzi, M., Wang, G., Weaverdyck, N., Weller, J., Whitehorn, N., Wu, W. L. K., Yefremenko, V., Young, M. R., and UAM. Departamento de Física Teórica
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Física, FOS: Physical sciences, XMM-newton Telescope, Galaxies, Cosmos, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We infer the mean optical depth of a sample of optically selected galaxy clusters from the Dark Energy Survey via the pairwise kinematic Sunyaev-Zel'dovich (KSZ) effect. The pairwise KSZ signal between pairs of clusters drawn from the Dark Energy Survey Year-3 cluster catalog is detected at 4.1 σ in cosmic microwave background temperature maps from two years of observations with the SPT-3G camera on the South Pole Telescope. After cuts, there are 24,580 clusters in the ∼1 ,400 deg2 of the southern sky observed by both experiments. We infer the mean optical depth of the cluster sample with two techniques. The optical depth inferred from the pairwise KSZ signal is τ¯e=(2.97 ±0.73 )×10-3 , while that inferred from the thermal SZ signal is τ¯e=(2.51 ±0.5 5stat±0.1 5syst)×10-3 . The two measures agree at 0.6 σ . We perform a suite of systematic checks to test the robustness of the analysis, The DES participants from Spanish institutions are partially E. SCHIAPPUCCI et al. PHYS. REV. D 107, 042004 (2023) 042004-14 supported by MICINN under Grants No. ESP2017-89838, No. PGC2018-094773, No. PGC2018-102021, No. SEV2016-0588, No. SEV-2016-0597, and No. MDM-2015- 0509, some of which include ERDF funds from the European Union. I. F. A. E. is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC Grant Agreements No. 240672, No. 291329, and No. 306478
Published: 2022
Full Text: View/download PDF

35. Dark Energy Survey Year 3 Results: Constraints on extensions to $Λ$CDM with weak lensing and galaxy clustering

Author: DES Collaboration, Abbott, T. M. C., Aguena, M., Alarcon, A., Alves, O., Amon, A., Annis, J., Avila, S., Bacon, D., Baxter, E., Bechtol, K., Becker, M. R., Bernstein, G. M., Birrer, S., Blazek, J., Bocquet, S., Brandao-Souza, A., Bridle, S. L., Brooks, D., Burke, D. L., Camacho, H., Campos, A., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Castander, F. J., Cawthon, R., Chang, C., Chen, A., Chen, R., Choi, A., Conselice, C., Cordero, J., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., Davis, C., Davis, T. M., DeRose, J., Desai, S., Di Valentino, E., Diehl, H. T., Dodelson, S., Doel, P., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Elvin-Poole, J., Everett, S., Fang, X., Farahi, A., Ferrero, I., Ferté, A., Flaugher, B., Fosalba, P., Friedel, D., Friedrich, O., Frieman, J., García-Bellido, J., Gatti, M., Giani, L., Giannantonio, T., Giannini, G., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hamaus, N., Harrison, I., Hartley, W. G., Herner, K., Hinton, S. R., Hollowood, D. L., Honscheid, K., Huang, H., Huff, E. M., Huterer, D., Jain, B., James, D. J., Jarvis, M., Jeffrey, N., Jeltema, T., Kovacs, A., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lee, S., Leget, P. -F., Lemos, P., Leonard, C. D., Liddle, A. R., Lima, M., Lin, H., MacCrann, N., Marshall, J. L., McCullough, J., Mena-Fernández, J., Menanteau, F., Miquel, R., Miranda, V., Mohr, J. J., Muir, J., Myles, J., Nadathur, S., Navarro-Alsina, A., Nichol, R. C., Ogando, R. L. C., Omori, Y., Palmese, A., Pandey, S., Park, Y., Paterno, M., Paz-Chinchón, F., Percival, W. J., Pieres, A., Malagón, A. A. Plazas, Porredon, A., Prat, J., Raveri, M., Rodriguez-Monroy, M., Rogozenski, P., Rollins, R. P., Romer, A. K., Roodman, A., Rosenfeld, R., Ross, A. J., Rykoff, E. S., Samuroff, S., Sánchez, C., Sanchez, E., Sanchez, J., Cid, D. Sanchez, Scarpine, V., Scolnic, D., Secco, L. F., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Smith, M., Soares-Santos, M., Suchyta, E., Tabbutt, M., Tarle, G., Thomas, D., To, C., Troja, A., Troxel, M. A., Tutusaus, I., Varga, T. N., Vincenzi, M., Walker, A. R., Weaverdyck, N., Wechsler, R. H., Weller, J., Yanny, B., Yin, B., Zhang, Y., and Zuntz, J.
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences
Abstract: We constrain extensions to the $Λ$CDM model using measurements from the Dark Energy Survey's first three years of observations and external data. The DES data are the two-point correlation functions of weak gravitational lensing, galaxy clustering, and their cross-correlation. We use simulated data and blind analyses of real data to validate the robustness of our results. In many cases, constraining power is limited by the absence of nonlinear predictions that are reliable at our required precision. The models are: dark energy with a time-dependent equation of state, non-zero spatial curvature, sterile neutrinos, modifications of gravitational physics, and a binned $σ_8(z)$ model which serves as a probe of structure growth. For the time-varying dark energy equation of state evaluated at the pivot redshift we find $(w_{\rm p}, w_a)= (-0.99^{+0.28}_{-0.17},-0.9\pm 1.2)$ at 68% confidence with $z_{\rm p}=0.24$ from the DES measurements alone, and $(w_{\rm p}, w_a)= (-1.03^{+0.04}_{-0.03},-0.4^{+0.4}_{-0.3})$ with $z_{\rm p}=0.21$ for the combination of all data considered. Curvature constraints of $Ω_k=0.0009\pm 0.0017$ and effective relativistic species $N_{\rm eff}=3.10^{+0.15}_{-0.16}$ are dominated by external data. For massive sterile neutrinos, we improve the upper bound on the mass $m_{\rm eff}$ by a factor of three compared to previous analyses, giving 95% limits of $(ΔN_{\rm eff},m_{\rm eff})\leq (0.28, 0.20\, {\rm eV})$. We also constrain changes to the lensing and Poisson equations controlled by functions $Σ(k,z) = Σ_0 Ω_Λ(z)/Ω_{Λ,0}$ and $μ(k,z)=μ_0 Ω_Λ(z)/Ω_{Λ,0}$ respectively to $Σ_0=0.6^{+0.4}_{-0.5}$ from DES alone and $(Σ_0,μ_0)=(0.04\pm 0.05,0.08^{+0.21}_{-0.19})$ for the combination of all data. Overall, we find no significant evidence for physics beyond $Λ$CDM., Updated to match published version. 46 pages, 25 figures, data available at https://dev.des.ncsa.illinois.edu/releases/y3a2/Y3key-extensions
Published: 2022
Full Text: View/download PDF

36. Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample

Author: Pandey, S., Krause, E., DeRose, J., MacCrann, N., Jain, B., Crocce, M., Blazek, J., Choi, A., Huang, H., To, C., Fang, X., Elvin-Poole, J., Prat, J., Porredon, A., Secco, L. F., Rodriguez-Monroy, M., Weaverdyck, N., Park, Y., Raveri, M., Rozo, E., Rykoff, E. S., Bernstein, G. M., Sánchez, C., Jarvis, M., Troxel, M. A., Zacharegkas, G., Chang, C., Alarcon, A., Alves, O., Amon, A., Andrade-Oliveira, F., Baxter, E., Bechtol, K., Becker, M. R., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Chen, R., Chintalapati, P., Davis, C., Di Valentino, E., Diehl, H. T., Dodelson, S., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Everett, S., Farahi, A., Ferté, A., Fosalba, P., Friedrich, O., Gatti, M., Giannini, G., Gruen, D., Gruendl, R. A., Harrison, I., Hartley, W. G., Huff, E. M., Huterer, D., Kovacs, A., Leget, P. F., McCullough, J., Muir, J., Myles, J., Navarro-Alsina, A., Omori, Y., Rollins, R. P., Roodman, A., Rosenfeld, R., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troja, A., Tutusaus, I., Varga, T. N., Wechsler, R. H., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Brooks, D., Burke, D. L., Carretero, J., Conselice, C., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Dietrich, J. P., Doel, P., Evrard, A. E., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Lin, H., Maia, M. A. G., Marshall, J. L., Melchior, P., Menanteau, F., Miller, C. J., Miquel, R., Mohr, J. J., Morgan, R., Palmese, A., Paz-Chinchón, F., Petravick, D., Pieres, A., Plazas Malagón, A. A., Sanchez, E., Scarpine, V., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., Weller, J., DES Collaboration, Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), DES, Department of Energy (US), National Science Foundation (US), Ministerio de Educación y Ciencia (España), Ministerio de Economía y Competitividad (España), Generalitat de Catalunya, Australian Research Council, European Commission, European Research Council, Pandey, S., Krause, E., Derose, J., Maccrann, N., Jain, B., Crocce, M., Blazek, J., Choi, A., Huang, H., To, C., Fang, X., Elvin-Poole, J., Prat, J., Porredon, A., Secco, L. F., Rodriguez-Monroy, M., Weaverdyck, N., Park, Y., Raveri, M., Rozo, E., Rykoff, E. S., Bernstein, G. M., Sánchez, C., Jarvis, M., Troxel, M. A., Zacharegkas, G., Chang, C., Alarcon, A., Alves, O., Amon, A., Andrade-Oliveira, F., Baxter, E., Bechtol, K., Becker, M. R., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Cawthon, R., Chen, R., Chintalapati, P., Davis, C., Di Valentino, E., Diehl, H. T., Dodelson, S., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Everett, S., Farahi, A., Ferté, A., Fosalba, P., Friedrich, O., Gatti, M., Giannini, G., Gruen, D., Gruendl, R. A., Harrison, I., Hartley, W. G., Huff, E. M., Huterer, D., Kovacs, A., Leget, P. F., Mccullough, J., Muir, J., Myles, J., Navarro-Alsina, A., Omori, Y., Rollins, R. P., Roodman, A., Rosenfeld, R., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troja, A., Tutusaus, I., Varga, T. N., Wechsler, R. H., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Brooks, D., Burke, D. L., Carretero, J., Conselice, C., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Dietrich, J. P., Doel, P., Evrard, A. E., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Jeltema, T., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Lin, H., Maia, M. A. G., Marshall, J. L., Melchior, P., Menanteau, F., Miller, C. J., Miquel, R., Mohr, J. J., Morgan, R., Palmese, A., Paz-Chinchón, F., Petravick, D., Pieres, A., Plazas Malagón, A. A., Sanchez, E., Scarpine, V., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., Weller, J., and Des, Collaboration
Subjects: Cosmology and Nongalactic Astrophysic, combination, Cosmology and Nongalactic Astrophysics (astro-ph.CO), challenge lightcone simulation, Astrophysics of Galaxies, FOS: Physical sciences, marginalization, Astrophysics, Cosmology and Nongalactic Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, calibration, Astrophysics - Astrophysics of Galaxies, efficient, Astrophysic, scale dependence, Astrophysics of Galaxies (astro-ph.GA), halo-mass, evolution, impact, redshift distributions, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: S. Pandey et al., We constrain cosmological parameters and galaxy-bias parameters using the combination of galaxy clustering and galaxy-galaxy lensing measurements from the Dark Energy Survey (DES) year-3 data. We describe our modeling framework and choice of scales analyzed, validating their robustness to theoretical uncertainties in small-scale clustering by analyzing simulated data. Using a linear galaxy-bias model and redMaGiC galaxy sample, we obtain 10% constraints on the matter density of the Universe. We also implement a nonlinear galaxy-bias model to probe smaller scales that includes parametrization based on hybrid perturbation theory and find that it leads to a 17% gain in cosmological constraining power. We perform robustness tests of our methodology pipeline and demonstrate stability of the constraints to changes in the theory model. Using the redMaGiC galaxy sample as foreground lens galaxies and adopting the best-fitting cosmological parameters from DES year-1 data, we find the galaxy clustering and galaxy-galaxy lensing measurements to exhibit significant signals akin to decorrelation between galaxies and mass on large scales, which is not expected in any current models. This likely systematic measurement error biases our constraints on galaxy bias and the S8 parameter. We find that a scale-, redshift- and sky-area-independent phenomenological decorrelation parameter can effectively capture this inconsistency between the galaxy clustering and galaxy-galaxy lensing. We trace the source of this correlation to a color-dependent photometric issue and minimize its impact on our result by changing the selection criteria of redMaGiC galaxies. Using this new sample, our constraints on the S8 parameter are consistent with previous studies and we find a small shift in the Ωm constraints compared to the fiducial redMaGiC sample. We infer the constraints on the mean host-halo mass of the redMaGiC galaxies in this new sample from the large-scale bias constraints, finding the galaxies occupy halos of mass approximately 1.6×1013M⊙/h., E. K. is supported by the Department of Energy Grant No. DE-SC0020247 and the David and Lucile Packard Foundation. S. P. and B.J. are supported in part by the U.S. Department of Energy Grant No. DE-SC0007901 and NASA ATP Grant No. NNH17ZDA001N. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at The OhioStateUniversity, theMitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministerio da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energ´eticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at UrbanaChampaign, the Institut de Ci`encies de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität MünchenandtheassociatedExcellenceCluster Universe,the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. The DES data management system is supported by the National Science Foundation under Grants No. AST-1138766 and No. AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under Grants No. AYA2015-71825, No. ESP2015-88861, No. FPA2015-68048, No. SEV-2012-0234, No. SEV-20160597, and No. MDM-2015-0509, some of which include ERDFfundsfromtheEuropean Union. I.F.A.E. is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/ 2007-2013) including ERC Grant Agreements No. 240672, No.291329,andNo.306478.Weacknowledgesupportfrom the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through Project No. CE110001020. This manuscript has been authored by Fermi Research Alliance, LLC under Contract No. DEAC02-07CH11359 with the U.S. Department of Energy, Office ofScience,OfficeofHighEnergyPhysics.
Published: 2021

37. Neuro-telehealth for fragile patients in a tertiary referral neurological institute during the COVID-19 pandemic in Milan, Lombardy

Author: Pareyson D., Pantaleoni C., Eleopra R., De Filippis G., Moroni I., Freri E., Zibordi F., Bulgheroni S., Pagliano E., Sarti D., Silvani A., Grazzi L., Tiraboschi P., Didato G., Anghileri E., Bersano A., Valentini L., Piacentini S., Muscio C., Leonardi M., Mariotti C., Eoli M., Nuzzo S., Tagliavini F., Confalonieri P., De Giorgi F., Antozzi C., Ardissone A., Bersano E., Boncoraglio G., Bonvegna S., Botturi A., Brambilla L., Canafoglia L., Caputi L., Caroppo P., Carriero M. R., Casali C., Casazza M., Catania A., Ciaccio C., Cilia R., DallaBella E., D'Amico D., Danti F. R., D'Arrigo S., DeCurtis M., Deleo F., Devigili G., DiFede G., DiGiacomo R., Elia A., Esposito S., Estienne M., Fenu S., Fichera M., Finocchiaro G., Frangiamore R., Gatti M., Gaviani P., Giaccone G., Giani L., Giovagnoli A. R., Andreasi N. G., Granata T., Granocchio E., Lamperti C., Lamperti E., Leone M., Masson R., Nanetti L., Nardocci N., Pastori C., Pisciotta C., Cecchini A. P., Ragona F., Redaelli V., Saletti V., Salsano E., Scelzo E., Solazzi R., Tozzo A., Usai S., Zorzi G., Arnoldi M. T., Foscan M., Marchi A., Pedrinelli I., Zanin R., Gazzola S., Magazu S., Scopelliti M. R., Casalino T., DeSalvatore M., Mazzanti S., Taddei M., Fedeli A., Sattin D., Galimberti L., Zagari R., Bombonato M., Fonte L., Floridia S., Pareyson, D, Pantaleoni, C, Eleopra, R, De Filippis, G, Moroni, I, Freri, E, Zibordi, F, Bulgheroni, S, Pagliano, E, Sarti, D, Silvani, A, Grazzi, L, Tiraboschi, P, Didato, G, Anghileri, E, Bersano, A, Valentini, L, Piacentini, S, Muscio, C, Leonardi, M, Mariotti, C, Eoli, M, Nuzzo, S, Tagliavini, F, Confalonieri, P, De Giorgi, F, Antozzi, C, Ardissone, A, Bersano, E, Boncoraglio, G, Bonvegna, S, Botturi, A, Brambilla, L, Canafoglia, L, Caputi, L, Caroppo, P, Carriero, M, Casali, C, Casazza, M, Catania, A, Ciaccio, C, Cilia, R, Dallabella, E, D'Amico, D, Danti, F, D'Arrigo, S, Decurtis, M, Deleo, F, Devigili, G, Difede, G, Digiacomo, R, Elia, A, Esposito, S, Estienne, M, Fenu, S, Fichera, M, Finocchiaro, G, Frangiamore, R, Gatti, M, Gaviani, P, Giaccone, G, Giani, L, Giovagnoli, A, Andreasi, N, Granata, T, Granocchio, E, Lamperti, C, Lamperti, E, Leone, M, Masson, R, Nanetti, L, Nardocci, N, Pastori, C, Pisciotta, C, Cecchini, A, Ragona, F, Redaelli, V, Saletti, V, Salsano, E, Scelzo, E, Solazzi, R, Tozzo, A, Usai, S, Zorzi, G, Arnoldi, M, Foscan, M, Marchi, A, Pedrinelli, I, Zanin, R, Gazzola, S, Magazu, S, Scopelliti, M, Casalino, T, Desalvatore, M, Mazzanti, S, Taddei, M, Fedeli, A, Sattin, D, Galimberti, L, Zagari, R, Bombonato, M, Fonte, L, and Floridia, S
Subjects: Adult, medicine.medical_specialty, Telemedicine, Neurology, Referral, Dermatology, Telehealth, 03 medical and health sciences, 0302 clinical medicine, Pandemic, medicine, Humans, Outpatient clinic, 030212 general & internal medicine, Medical prescription, Child, Pandemics, Referral and Consultation, SARS-CoV-2, business.industry, Teleneurorehabilitation, COVID-19, General Medicine, medicine.disease, Televisit, Psychiatry and Mental health, Italy, Neuro-telehealth, Neurology (clinical), Neurosurgery, Medical emergency, business, 030217 neurology & neurosurgery
Abstract: Background: Lombardy was severely hit by the COVID-19 pandemic since February 2020 and the Health System underwent rapid reorganization. Outpatient clinics were stopped for non-urgent patients: it became a priority to manage hundreds of fragile neurological patients who suddenly had less reference points. In Italy, before the pandemic, Televisits were neither recognized nor priced. Methods: At the Fondazione IRCCS Istituto Neurologico C. Besta, we reorganized outpatient clinics to deliver Neuro-telemedicine services, including Televisits and Teleneurorehabilitation, since March 2020. A dedicated Working Group prepared the procedure, tested the system, and designed satisfaction questionnaires for adults and children. Results: After a pilot phase, we prepared a procedure for Telemedicine outpatient clinics which was approved by hospital directions. It included prescription, booking, consenting, privacy and data protection, secure connection with patients (Teams Microsoft 365), electronic report preparation and delivery, reporting, and accountability of the services. During the March–September 2020 period, we delivered 3167 Telemedicine services, including 1618 Televisits, to 1694 patients (972 adults, 722 children) with a wide range of chronic neurological disorders. We successfully administered different clinical assessment and scales. Satisfaction among patients and caregivers was very high. Conclusions: During the dramatic emergency, we were able to take care of more than 1600 patients by organizing Neuro-telehealth in a few weeks, lessening the impact of the pandemic on fragile patients with chronic neurological disorders; this strategy is now stably embedded in our care pathways. In Italy, Telehealth is at present recognized and priced and is becoming a stable pillar of the health system.
Published: 2021

38. Impact of COVID-19 on the imaging diagnosis of cardiac disease in Europe

Author: Williams M. C., Shaw L., Hirschfeld C. B., Maurovich-Horvat P., Norgaard B. L., Pontone G., Jimenez-Heffernan A., Sinitsyn V., Sergienko V., Ansheles A., Bax J. J., Buechel R., Milan E., Slart R. H. J. A., Nicol E., Bucciarelli-Ducci C., Pynda Y., Better N., Cerci R., Dorbala S., Raggi P., Villines T. C., Vitola J., Malkovskiy E., Goebel B., Cohen Y., Randazzo M., Pascual T. N. B., Dondi M., Paez D., Einstein A. J., Nasery M. N., Goda A., Shirka E., Benlabgaa R., Bouyoucef S., Medjahedi A., Nailli Q., Agolti M., Aguero R. N., Del Carmen Alak M., Alberguina L. G., Arronada G., Astesiano A., Norton C. B., Benteo P., Blanco J., Bonelli J. M., Bustos J. J., Cabrejas R., Cachero J., Campisi R., Canderoli A., Carames S., Carrascosa P., Castro R., Cendoya O., Cognigni L. M., Collaud C., Cortes C., Courtis J., Cragnolino D., Daicz M., De La Vega A., De Maria S. T., Del Riego H., Dettori F., Deviggiano A., Dragonetti L., Embon M., Enriquez R. E., Ensinas J., Faccio F., Facello A., Garofalo D., Geronazzo R., Gonza N., Gutierrez L., Guzzo M. A., Hasbani V., Huerin M., Jager V., Lewkowicz J. M., De Munain M. N. A. L., Lotti J. M., Marquez A., Masoli O., Masoli O. H., Mastrovito E., Mayoraz M., Melado G. E., Mele A., Merani M. F., Meretta A. H., Molteni S., Montecinos M., Noguera E., Novoa C., Sueldo C. P., Ascani S. P., Pollono P., Pujol M. P., Radzinschi A., Raimondi G., Redruello M., Rodriguez M., Romero R. L., Acuna A. R., Rovaletti F., Miguel L. S., Solari L., Strada B., Traverso S., Traverzo S. S., Del Huerto Velazquez Espeche M., Weihmuller J. S., Wolcan J., Zeffiro S., Sakanyan M., Beuzeville S., Boktor R., Butler P., Calcott J., Carr L., Chan V., Chao C., Chong W., Dobson M., Downie D., Dwivedi G., Elison B., Engela J., Francis R., Gaikwad A., Basavaraj A. G., Goodwin B., Greenough R., Hamilton-Craig C., Hsieh V., Joshi S., Lederer K., Lee K., Lee J., Magnussen J., Mai N., Mander G., Murton F., Nandurkar D., Neill J., O'Rourke E., O'Sullivan P., Pandos G., Pathmaraj K., Pitman A., Poulter R., Premaratne M., Prior D., Ridley L., Rutherford N., Salehi H., Saunders C., Scarlett L., Seneviratne S., Shetty D., Shrestha G., Shulman J., Solanki V., Stanton T., Stuart M., Stubbs M., Swainson I., Taubman K., Taylor A., Thomas P., Unger S., Upton A., Vamadevan S., Van Gaal W., Verjans J., Voutnis D., Wayne V., Wilson P., Wong D., Wong K., Younger J., Feuchtner G., Mirzaei S., Weiss K., Maroz-Vadalazhskaya N., Gheysens O., Homans F., Moreno-Reyes R., Pasquet A., Roelants V., Van De Heyning C. M., Rios R. A., Soldat-Stankovic V., Stankovic S., Siqueira M. H. A., Almeida A., Togni P. H. A., Andrade J. H., Andrade L., Anselmi C., Araujo R., Azevedo G., Bezerra S., Biancardi R., Grossman G. B., Brandao S., Pianta D. B., Carreira L., Castro B., Chang T., Cunali F., Cury R., Dantas R., De Amorim Fernandes F., De Lorenzo A., De MacEdo Filho R., Erthal F., Fernandes F., Fernandes J., De Souza T. F., Alves W. F., Ghini B., Goncalves L., Gottlieb I., Hadlich M., Kameoka V., Lima R., Lima A., Lopes R. W., E Silva R. M., Magalhaes T., Silva F. M., Mastrocola L. E., Medeiros F., Meneghetti J. C., Naue V., Naves D., Nolasco R., Nomura C., Oliveira J. B., Paixao E., De Carvalho F. P., Pinto I., Possetti P., Quinta M., Ramos R. R. N., Rocha R., Rodrigues A., Rodrigues C., Romantini L., Sanches A., Santana S., Da Silva L. S., Schvartzman P., Matushita C. S., Senra T., Shiozaki A., De Siqueira M. E. M., Siqueira C., Smanio P., Soares C. E., Soares J., Bittencourt M. S., Spiro B., Mesquita C. T., Torreao J., Torres R., Uellendahl M., Monte G. U., Verissimo O., Cabeda E. V., Pedras F. V., Waltrick R., Zapparoli M., Naseer H., Garcheva-Tsacheva M., Kostadinova I., Theng Y., Abikhzer G., Barette R., Chow B., Dabreo D., Friedrich M., Garg R., Hafez M. N., Johnson C., Kiess M., Leipsic J., Leung E., Miller R., Oikonomou A., Probst S., Roifman I., Small G., Tandon V., Trivedi A., White J., Zukotynski K., Canessa J., Munoz G. C., Concha C., Hidalgo P., Lovera C., Massardo T., Vargas L. S., Abad P., Arturo H., Ayala S., Benitez L., Cadena A., Caicedo C., Moncayo A. C., Gomez S., Villamil C. T. G., Jaimes C., Londono J., Blair J. L. L., Pabon L., Pineda M., Rojas J. C., Ruiz D., Escobar M. V., Vasquez A., Vergel D., Zuluaga A., Gamboa I. B., Castro G., Gonzalez U., Baric A., Batinic T., Franceschi M., Hrabak M., Jukic M., Medakovic P., Persic V., Prpic M., Punda A., Batista J. F., Lauchy J. M. G., Gutierrez Y. M., Menendez R., Peix A., Rochela L., Panagidis C., Petrou I., Engelmann V., Kaminek M., Kincl V., Lang O., Simanek M., Abdulla J., Bottcher M., Christensen M., Gormsen L. C., Hasbak P., Hess S., Holdgaard P., Johansen A., Kyhl K., Ovrehus K. A., Sand N. P. R., Steffensen R., Thomassen A., Zerahn B., Perez A., Velez G. A. E., Velez M. S., Aziz I. S. A., Abougabal M., Ahmed T., Allam A., Asfour A., Hassan M., Hassan A., Ibrahim A., Kaffas S., Kandeel A., Ali M. M., Mansy A., Maurice H., Nabil S., Shaaban M., Flores A. C., Poksi A., Knuuti J., Kokkonen V., Larikka M., Uusitalo V., Bailly M., Burg S., Deux J. -F., Habouzit V., Hyafil F., Lairez O., Proffit F., Regaieg H., Sarda-Mantel L., Tacher V., Schneider R. P., Ayetey H., Angelidis G., Archontaki A., Chatziioannou S., Datseris I., Fragkaki C., Georgoulias P., Koukouraki S., Koutelou M., Kyrozi E., Repasos E., Stavrou P., Valsamaki P., Gonzalez C., Gutierrez G., Maldonado A., Buga K., Garai I., Schmidt E., Szilveszter B., Varady E., Banthia N., Bhagat J. K., Bhargava R., Bhat V., Bhatia M., Choudhury P., Chowdekar V. S., Irodi A., Jain S., Joseph E., Kumar S., Mahapatra G., Mitra D., Mittal B. R., Ozair A., Patel C., Patel T., Patel R., Patel S., Saxena S., Sengupta S., Singh S., Singh B., Sood A., Verma A., Affandi E., Alam P. S., Edison E., Gunawan G., Hapkido H., Hidayat B., Huda A., Mukti A. P., Prawiro D., Soeriadi E. A., Syawaluddin H., Albadr A., Assadi M., Emami F., Houshmand G., Maleki M., Rostami M. T., Zakavi S. R., Zaid E. A., Agranovich S., Arnson Y., Bar-Shalom R., Frenkel A., Knafo G., Lugassi R., Moalem I. S. M., Mor M., Muskal N., Ranser S., Shalev A., Albano D., Alongi P., Arnone G., Bagatin E., Baldari S., Bauckneht M., Bertelli P., Bianco F., Bonfiglioli R., Boni R., Bruno A., Bruno I., Busnardo E., Califaretti E., Camoni L., Carnevale A., Casoni R., Cavallo A. U., Cavenaghi G., Chierichetti F., Chiocchi M., Cittanti C., Colletta M., Conti U., Cossu A., Cuocolo A., Cuzzocrea M., De Rimini M. L., De Vincentis G., Del Giudice E., Del Torto A., Della Tommasina V., Durmo R., Erba P. A., Evangelista L., Faletti R., Faragasso E., Farsad M., Ferro P., Florimonte L., Frantellizzi V., Fringuelli F. M., Gatti M., Gaudiano A., Gimelli A., Giubbini R., Giuffrida F., Ialuna S., Laudicella R., Leccisotti L., Leva L., Liga R., Liguori C., Longo G., Maffione M., Mancini M. E., Marcassa C., Nardi B., Pacella S., Pepe G., Pulizzi S., Quartuccio N., Rampin L., Ricci F., Rossini P., Rubini G., Russo V., Sacchetti G. M., Sambuceti G., Scarano M., Sciagra R., Sperandio M., Stefanelli A., Ventroni G., Zoboli S., Baugh D., Chambers D., Madu E., Nunura F., Asano H., Chimura C. M., Fujimoto S., Fujisue K., Fukunaga T., Fukushima Y., Fukuyama K., Hashimoto J., Ichikawa Y., Iguchi N., Imai M., Inaki A., Ishimura H., Isobe S., Kadokami T., Kato T., Kudo T., Kumita S., Maruno H., Mataki H., Miyagawa M., Morimoto R., Moroi M., Nagamachi S., Nakajima K., Nakata T., Nakazato R., Nanasato M., Naya M., Norikane T., Ohta Y., Okayama S., Okizaki A., Otomi Y., Otsuka H., Saito M., Sakata S. Y., Sarai M., Sato D., Shiraishi S., Suwa Y., Takanami K., Takehana K., Taki J., Tamaki N., Taniguchi Y., Teragawa H., Tomizawa N., Tsujita K., Umeji K., Wakabayashi Y., Yamada S., Yamazaki S., Yoneyama T., Rawashdeh M., Batyrkhanov D., Dautov T., Makhdomi K., Ombati K., Alkandari F., Garashi M., Coie T. L., Rajvong S., Kalinin A., Kalnina M., Haidar M., Komiagiene R., Kviecinskiene G., Mataciunas M., Vajauskas D., Picard C., Karim N. K. A., Reichmuth L., Samuel A., Allarakha M. A., Naojee A. S., Alexanderson-Rosas E., Barragan E., Becerril A., Gonzalez-Montecinos, Cabada M., Rodriguez D. C., Carvajal-Juarez I., Cortes V., Cortes F., De La Pena E., Gama-Moreno M., Gonzalez L., Ramirez N. G., Jimenez-Santos M., Matos L., Monroy E., Morelos M., Ornelas M., Ramirez J. A. O., Preciado-Anaya A., Preciado-Gutierrez O. U., Barragan A. P., Uvera S. G. R., Sandoval S., Tomas M. S., Sierra-Galan L. M., Siu S., Vallejo E., Valles M., Faraggi M., Sereegotov E., Ilic S., Ben-Rais N., Alaoui N. I., Taleb S., Myo K. P. P., Thu P. S., Ghimire R. K., Rajbanshi B., Barneveld P., Glaudemans A., Habets J., Koopmans K. P., Manders J., Pool S., Scholte A., Scholtens A., Slart R., Thimister P., Van Asperen E. -J., Veltman N., Verschure D., Wagenaar N., Edmond J., Ellis C., Johnson K., Keenan R., Kueh S. H., Occleshaw C., Sasse A., To A., Van Pelt N., Young C., Cuadra T., Vanegas H. B. R., Soli I. A., Issoufou D. M., Ayodele T., Madu C., Onimode Y., Efros-Monsen E., Forsdahl S. H., Dimmen J. -M. H., Jorgensen A., Krohn I., Lovhaugen P., Braten A. T., Al Dhuhli H., Al Kindi F., Al-Bulushi N., Jawa Z., Tag N., Afzal M. S., Fatima S., Younis M. N., Riaz M., Saadullah M., Herrera Y., Lenturut-Katal D., Vazquez M. C., Ortellado J., Akhter A., Cao D., Cheung S., Dai X., Gong L., Han D., Hou Y., Li C., Li T., Li D., Li S., Liu J., Liu H., Lu B., Ng M. Y., Sun K., Tang G., Wang J., Wang X., Wang Z. -Q., Wang Y., Wu J., Wu Z., Xia L., Xiao J., Xu L., Yang Y., Yin W., Yu J., Yuan L., Zhang T., Zhang L., Zhang Y. -G., Zhang X., Zhu L., Alfaro A., Abrihan P., Barroso A., Cruz E., Gomez M. R., Magboo V. P., Medina J. M., Obaldo J., Pastrana D., Pawhay C. M., Quinon A., Tang J. M., Tecson B., Uson K. J., Uy M., Kostkiewicz M., Kunikowska J., Bettencourt N., Cantinho G., Ferreira A., Syed G., Arnous S., Atyani S., Byrne A., Gleeson T., Kerins D., Meehan C., Murphy D., Murphy M., Murray J., O'Brien J., Bang J. -I., Bom H., Cho S. -G., Hong C. M., Jang S. J., Jeong Y. H., Kang W. J., Kim J. -Y., Namgung C. K., So Y., Won K. S., Majstorov V., Vavlukis M., Salobir B. G., Stalc M., Benedek T., Benedek I., Mititelu R., Stan C. A., Dariy O., Drozdova O., Gagarina N., Gulyaev V. M., Itskovich I., Karalkin A., Kokov A., Migunova E., Pospelov V., Ryzhkova D., Saifullina G., Sazonova S., Shurupova I., Trifonova T., Ussov W. Y., Vakhromeeva M., Valiullina N., Zavadovsky K., Zhuravlev K., Alasnag M., Okarvi S., Saranovic D. S., Keng F., See J. H. J., Sekar R., Yew M. S., Vondrak A., Bejai S., Bennie G., Bester R., Engelbrecht G., Evbuomwan O., Gongxeka H., Vuuren M. J., Kaplan M., Khushica P., Lakhi H., Louw L., Malan N., Milos K., Modiselle M., More S., Naidoo M., Scholtz L., Vangu M., Aguade-Bruix S., Blanco I., Cabrera A., Camarero A., Casans-Tormo I., Cuellar-Calabria H., Flotats A., Canamero M. E. F., Garcia M. E., Leta R., Diaz J. L., Lumbreras L., Marquez-Cabeza J. J., Martin F., De Alegria A. M., Medina F., Canal M. P., Peiro V., Pubul-Nunez V., Madrid J. I. R., Rey C. R., Perez R. R., Ruiz J., Hernandez G. S., Sevilla A., Zeidan N., Nanayakkara D., Udugama C., Simonsson M., Alkadhi H., Buechel R. R., Burger P., Ceriani L., De Boeck B., Grani C., De Saint Lager Lucas A. J., Kamani C. H., Kawel-Boehm N., Manka R., Prior J. O., Rominger A., Vallee J. -P., Khiewvan B., Premprabha T., Thientunyakit T., Sellem A., Kir K. M., Sayman H., Sebikali M. J., Muyinda Z., Kmetyuk Y., Korol P., Mykhalchenko O., Pliatsek V., Satyr M., Albalooshi B., Hassan M. I. A., Anderson J., Bedi P., Biggans T., Bularga A., Bull R., Burgul R., Carpenter J. -P., Coles D., Cusack D., Deshpande A., Dougan J., Fairbairn T., Farrugia A., Gopalan D., Gummow A., Ramkumar P. G., Hamilton M., Harbinson M., Hartley T., Hudson B., Joshi N., Kay M., Kelion A., Khokhar A., Kitt J., Low C., Mak S. M., Marousa N., Martin J., McAlindon E., Menezes L., Morgan-Hughes G., Moss A., Murray A., Patel D., Peebles C., Pugliese F., Rodrigues J. C. L., Rofe C., Sabharwal N., Schofield R., Semple T., Sharma N., Strouhal P., Subedi D., Topping W., Tweed K., Weir-Mccall J., Abbara S., Abbasi T., Abbott B., Abohashem S., Abramson S., Al-Abboud T., Al-Mallah M., Almousalli O., Ananthasubramaniam K., Kumar M. A., Askew J., Attanasio L., Balmer-Swain M., Bayer R. R., Bernheim A., Bhatti S., Bieging E., Blankstein R., Bloom S., Blue S., Bluemke D., Borges A., Branch K., Bravo P., Brothers J., Budoff M., Bullock-Palmer R., Burandt A., Burke F. W., Bush K., Candela C., Capasso E., Cavalcante J., Chang D., Chatterjee S., Chatzizisis Y., Cheezum M., Chen T., Chen J., Chen M., Choi A., Clarcq J., Cordero A., Crim M., Danciu S., Decter B., Dhruva N., Doherty N., Doukky R., Dunbar A., Duvall W., Edwards R., Esquitin K., Farah H., Fentanes E., Ferencik M., Fisher D., Fitzpatrick D., Foster C., Fuisz T., Gannon M., Gastner L., Gerson M., Ghoshhajra B., Goldberg A., Goldner B., Gonzalez J., Gore R., Gracia-Lopez S., Hage F., Haider A., Haider S., Hamirani Y., Hassen K., Hatfield M., Hawkins C., Hawthorne K., Heath N., Hendel R., Hernandez P., Hill G., Horgan S., Huffman J., Hurwitz L., Iskandrian A., Janardhanan R., Jellis C., Jerome S., Kalra D., Kaviratne S., Kay F., Kelly F., Khalique O., Kinkhabwala M., Iii G. K., Kircher J., Kirkbride R., Kontos M., Kottam A., Krepp J., Layer J., Lee S. H., Leppo J., Lesser J., Leung S., Lewin H., Litmanovich D., Liu Y., Lopez-Mattei J., Magurany K., Markowitz J., Marn A., Matis S. E., McKenna M., McRae T., Mendoza F., Merhige M., Min D., Moffitt C., Moncher K., Moore W., Morayati S., Morris M., Mossa-Basha M., Mrsic Z., Murthy V., Nagpal P., Napier K., Narula J., Nelson K., Nijjar P., Osman M., Parwani P., Passen E., Patel A., Patil P., Paul R., Phillips L., Polsani V., Poludasu R., Pomerantz B., Porter T., Prentice R., Pursnani A., Rabbat M., Ramamurti S., Rich F., Luna H. R., Robinson A., Robles K., Rodriguez C., Rorie M., Rumberger J., Russell R., Sabra P., Sadler D., Schemmer M., Schoepf U. J., Shah S., Shah N., Shanbhag S., Sharma G., Shayani S., Shirani J., Shivaram P., Sigman S., Simon M., Slim A., Smith D., Smith A., Soman P., Srichai-Parsia M. B., Streeter J., Albert T., Tawakol A., Thomas D., Thompson R., Torbet T., Trinidad D., Ullery S., Unzek S., Uretsky S., Vallurupalli S., Verma V., Waller A., Wang E., Ward P., Weissman G., Wesbey G., White K., Winchester D., Wolinsky D., Yost S., Zgaljardic M., Alonso O., Beretta M., Ferrando R., Kapitan M., Mut F., Djuraev O., Rozikhodjaeva G., Ngoc H. L., Mai S. H., Nguyen X. C., Williams, M, Shaw, L, Hirschfeld, C, Maurovich-Horvat, P, Norgaard, B, Pontone, G, Jimenez-Heffernan, A, Sinitsyn, V, Sergienko, V, Ansheles, A, Bax, J, Buechel, R, Milan, E, Slart, R, Nicol, E, Bucciarelli-Ducci, C, Pynda, Y, Better, N, Cerci, R, Dorbala, S, Raggi, P, Villines, T, Vitola, J, Malkovskiy, E, Goebel, B, Cohen, Y, Randazzo, M, Pascual, T, Dondi, M, Paez, D, Einstein, A, Nasery, M, Goda, A, Shirka, E, Benlabgaa, R, Bouyoucef, S, Medjahedi, A, Nailli, Q, Agolti, M, Aguero, R, Del Carmen Alak, M, Alberguina, L, Arronada, G, Astesiano, A, Norton, C, Benteo, P, Blanco, J, Bonelli, J, Bustos, J, Cabrejas, R, Cachero, J, Campisi, R, Canderoli, A, Carames, S, Carrascosa, P, Castro, R, Cendoya, O, Cognigni, L, Collaud, C, Cortes, C, Courtis, J, Cragnolino, D, Daicz, M, De La Vega, A, De Maria, S, Del Riego, H, Dettori, F, Deviggiano, A, Dragonetti, L, Embon, M, Enriquez, R, Ensinas, J, Faccio, F, Facello, A, Garofalo, D, Geronazzo, R, Gonza, N, Gutierrez, L, Guzzo, M, Hasbani, V, Huerin, M, Jager, V, Lewkowicz, J, De Munain, M, Lotti, J, Marquez, A, Masoli, O, Mastrovito, E, Mayoraz, M, Melado, G, Mele, A, Merani, M, Meretta, A, Molteni, S, Montecinos, M, Noguera, E, Novoa, C, Sueldo, C, Ascani, S, Pollono, P, Pujol, M, Radzinschi, A, Raimondi, G, Redruello, M, Rodriguez, M, Romero, R, Acuna, A, Rovaletti, F, Miguel, L, Solari, L, Strada, B, Traverso, S, Traverzo, S, Del Huerto Velazquez Espeche, M, Weihmuller, J, Wolcan, J, Zeffiro, S, Sakanyan, M, Beuzeville, S, Boktor, R, Butler, P, Calcott, J, Carr, L, Chan, V, Chao, C, Chong, W, Dobson, M, Downie, D, Dwivedi, G, Elison, B, Engela, J, Francis, R, Gaikwad, A, Basavaraj, A, Goodwin, B, Greenough, R, Hamilton-Craig, C, Hsieh, V, Joshi, S, Lederer, K, Lee, K, Lee, J, Magnussen, J, Mai, N, Mander, G, Murton, F, Nandurkar, D, Neill, J, O'Rourke, E, O'Sullivan, P, Pandos, G, Pathmaraj, K, Pitman, A, Poulter, R, Premaratne, M, Prior, D, Ridley, L, Rutherford, N, Salehi, H, Saunders, C, Scarlett, L, Seneviratne, S, Shetty, D, Shrestha, G, Shulman, J, Solanki, V, Stanton, T, Stuart, M, Stubbs, M, Swainson, I, Taubman, K, Taylor, A, Thomas, P, Unger, S, Upton, A, Vamadevan, S, Van Gaal, W, Verjans, J, Voutnis, D, Wayne, V, Wilson, P, Wong, D, Wong, K, Younger, J, Feuchtner, G, Mirzaei, S, Weiss, K, Maroz-Vadalazhskaya, N, Gheysens, O, Homans, F, Moreno-Reyes, R, Pasquet, A, Roelants, V, Van De Heyning, C, Rios, R, Soldat-Stankovic, V, Stankovic, S, Siqueira, M, Almeida, A, Togni, P, Andrade, J, Andrade, L, Anselmi, C, Araujo, R, Azevedo, G, Bezerra, S, Biancardi, R, Grossman, G, Brandao, S, Pianta, D, Carreira, L, Castro, B, Chang, T, Cunali, F, Cury, R, Dantas, R, De Amorim Fernandes, F, De Lorenzo, A, De MacEdo Filho, R, Erthal, F, Fernandes, F, Fernandes, J, De Souza, T, Alves, W, Ghini, B, Goncalves, L, Gottlieb, I, Hadlich, M, Kameoka, V, Lima, R, Lima, A, Lopes, R, E Silva, R, Magalhaes, T, Silva, F, Mastrocola, L, Medeiros, F, Meneghetti, J, Naue, V, Naves, D, Nolasco, R, Nomura, C, Oliveira, J, Paixao, E, De Carvalho, F, Pinto, I, Possetti, P, Quinta, M, Ramos, R, Rocha, R, Rodrigues, A, Rodrigues, C, Romantini, L, Sanches, A, Santana, S, Da Silva, L, Schvartzman, P, Matushita, C, Senra, T, Shiozaki, A, De Siqueira, M, Siqueira, C, Smanio, P, Soares, C, Soares, J, Bittencourt, M, Spiro, B, Mesquita, C, Torreao, J, Torres, R, Uellendahl, M, Monte, G, Verissimo, O, Cabeda, E, Pedras, F, Waltrick, R, Zapparoli, M, Naseer, H, Garcheva-Tsacheva, M, Kostadinova, I, Theng, Y, Abikhzer, G, Barette, R, Chow, B, Dabreo, D, Friedrich, M, Garg, R, Hafez, M, Johnson, C, Kiess, M, Leipsic, J, Leung, E, Miller, R, Oikonomou, A, Probst, S, Roifman, I, Small, G, Tandon, V, Trivedi, A, White, J, Zukotynski, K, Canessa, J, Munoz, G, Concha, C, Hidalgo, P, Lovera, C, Massardo, T, Vargas, L, Abad, P, Arturo, H, Ayala, S, Benitez, L, Cadena, A, Caicedo, C, Moncayo, A, Gomez, S, Villamil, C, Jaimes, C, Londono, J, Blair, J, Pabon, L, Pineda, M, Rojas, J, Ruiz, D, Escobar, M, Vasquez, A, Vergel, D, Zuluaga, A, Gamboa, I, Castro, G, Gonzalez, U, Baric, A, Batinic, T, Franceschi, M, Hrabak, M, Jukic, M, Medakovic, P, Persic, V, Prpic, M, Punda, A, Batista, J, Lauchy, J, Gutierrez, Y, Menendez, R, Peix, A, Rochela, L, Panagidis, C, Petrou, I, Engelmann, V, Kaminek, M, Kincl, V, Lang, O, Simanek, M, Abdulla, J, Bottcher, M, Christensen, M, Gormsen, L, Hasbak, P, Hess, S, Holdgaard, P, Johansen, A, Kyhl, K, Ovrehus, K, Sand, N, Steffensen, R, Thomassen, A, Zerahn, B, Perez, A, Velez, G, Velez, M, Aziz, I, Abougabal, M, Ahmed, T, Allam, A, Asfour, A, Hassan, M, Hassan, A, Ibrahim, A, Kaffas, S, Kandeel, A, Ali, M, Mansy, A, Maurice, H, Nabil, S, Shaaban, M, Flores, A, Poksi, A, Knuuti, J, Kokkonen, V, Larikka, M, Uusitalo, V, Bailly, M, Burg, S, Deux, J, Habouzit, V, Hyafil, F, Lairez, O, Proffit, F, Regaieg, H, Sarda-Mantel, L, Tacher, V, Schneider, R, Ayetey, H, Angelidis, G, Archontaki, A, Chatziioannou, S, Datseris, I, Fragkaki, C, Georgoulias, P, Koukouraki, S, Koutelou, M, Kyrozi, E, Repasos, E, Stavrou, P, Valsamaki, P, Gonzalez, C, Gutierrez, G, Maldonado, A, Buga, K, Garai, I, Schmidt, E, Szilveszter, B, Varady, E, Banthia, N, Bhagat, J, Bhargava, R, Bhat, V, Bhatia, M, Choudhury, P, Chowdekar, V, Irodi, A, Jain, S, Joseph, E, Kumar, S, Mahapatra, G, Mitra, D, Mittal, B, Ozair, A, Patel, C, Patel, T, Patel, R, Patel, S, Saxena, S, Sengupta, S, Singh, S, Singh, B, Sood, A, Verma, A, Affandi, E, Alam, P, Edison, E, Gunawan, G, Hapkido, H, Hidayat, B, Huda, A, Mukti, A, Prawiro, D, Soeriadi, E, Syawaluddin, H, Albadr, A, Assadi, M, Emami, F, Houshmand, G, Maleki, M, Rostami, M, Zakavi, S, Zaid, E, Agranovich, S, Arnson, Y, Bar-Shalom, R, Frenkel, A, Knafo, G, Lugassi, R, Moalem, I, Mor, M, Muskal, N, Ranser, S, Shalev, A, Albano, D, Alongi, P, Arnone, G, Bagatin, E, Baldari, S, Bauckneht, M, Bertelli, P, Bianco, F, Bonfiglioli, R, Boni, R, Bruno, A, Bruno, I, Busnardo, E, Califaretti, E, Camoni, L, Carnevale, A, Casoni, R, Cavallo, A, Cavenaghi, G, Chierichetti, F, Chiocchi, M, Cittanti, C, Colletta, M, Conti, U, Cossu, A, Cuocolo, A, Cuzzocrea, M, De Rimini, M, De Vincentis, G, Del Giudice, E, Del Torto, A, Della Tommasina, V, Durmo, R, Erba, P, Evangelista, L, Faletti, R, Faragasso, E, Farsad, M, Ferro, P, Florimonte, L, Frantellizzi, V, Fringuelli, F, Gatti, M, Gaudiano, A, Gimelli, A, Giubbini, R, Giuffrida, F, Ialuna, S, Laudicella, R, Leccisotti, L, Leva, L, Liga, R, Liguori, C, Longo, G, Maffione, M, Mancini, M, Marcassa, C, Nardi, B, Pacella, S, Pepe, G, Pulizzi, S, Quartuccio, N, Rampin, L, Ricci, F, Rossini, P, Rubini, G, Russo, V, Sacchetti, G, Sambuceti, G, Scarano, M, Sciagra, R, Sperandio, M, Stefanelli, A, Ventroni, G, Zoboli, S, Baugh, D, Chambers, D, Madu, E, Nunura, F, Asano, H, Chimura, C, Fujimoto, S, Fujisue, K, Fukunaga, T, Fukushima, Y, Fukuyama, K, Hashimoto, J, Ichikawa, Y, Iguchi, N, Imai, M, Inaki, A, Ishimura, H, Isobe, S, Kadokami, T, Kato, T, Kudo, T, Kumita, S, Maruno, H, Mataki, H, Miyagawa, M, Morimoto, R, Moroi, M, Nagamachi, S, Nakajima, K, Nakata, T, Nakazato, R, Nanasato, M, Naya, M, Norikane, T, Ohta, Y, Okayama, S, Okizaki, A, Otomi, Y, Otsuka, H, Saito, M, Sakata, S, Sarai, M, Sato, D, Shiraishi, S, Suwa, Y, Takanami, K, Takehana, K, Taki, J, Tamaki, N, Taniguchi, Y, Teragawa, H, Tomizawa, N, Tsujita, K, Umeji, K, Wakabayashi, Y, Yamada, S, Yamazaki, S, Yoneyama, T, Rawashdeh, M, Batyrkhanov, D, Dautov, T, Makhdomi, K, Ombati, K, Alkandari, F, Garashi, M, Coie, T, Rajvong, S, Kalinin, A, Kalnina, M, Haidar, M, Komiagiene, R, Kviecinskiene, G, Mataciunas, M, Vajauskas, D, Picard, C, Karim, N, Reichmuth, L, Samuel, A, Allarakha, M, Naojee, A, Alexanderson-Rosas, E, Barragan, E, Becerril, A, Gonzalez-Montecinos, Cabada, M, Rodriguez, D, Carvajal-Juarez, I, Cortes, V, Cortes, F, De La Pena, E, Gama-Moreno, M, Gonzalez, L, Ramirez, N, Jimenez-Santos, M, Matos, L, Monroy, E, Morelos, M, Ornelas, M, Ramirez, J, Preciado-Anaya, A, Preciado-Gutierrez, O, Barragan, A, Uvera, S, Sandoval, S, Tomas, M, Sierra-Galan, L, Siu, S, Vallejo, E, Valles, M, Faraggi, M, Sereegotov, E, Ilic, S, Ben-Rais, N, Alaoui, N, Taleb, S, Myo, K, Thu, P, Ghimire, R, Rajbanshi, B, Barneveld, P, Glaudemans, A, Habets, J, Koopmans, K, Manders, J, Pool, S, Scholte, A, Scholtens, A, Thimister, P, Van Asperen, E, Veltman, N, Verschure, D, Wagenaar, N, Edmond, J, Ellis, C, Johnson, K, Keenan, R, Kueh, S, Occleshaw, C, Sasse, A, To, A, Van Pelt, N, Young, C, Cuadra, T, Vanegas, H, Soli, I, Issoufou, D, Ayodele, T, Madu, C, Onimode, Y, Efros-Monsen, E, Forsdahl, S, Dimmen, J, Jorgensen, A, Krohn, I, Lovhaugen, P, Braten, A, Al Dhuhli, H, Al Kindi, F, Al-Bulushi, N, Jawa, Z, Tag, N, Afzal, M, Fatima, S, Younis, M, Riaz, M, Saadullah, M, Herrera, Y, Lenturut-Katal, D, Vazquez, M, Ortellado, J, Akhter, A, Cao, D, Cheung, S, Dai, X, Gong, L, Han, D, Hou, Y, Li, C, Li, T, Li, D, Li, S, Liu, J, Liu, H, Lu, B, Ng, M, Sun, K, Tang, G, Wang, J, Wang, X, Wang, Z, Wang, Y, Wu, J, Wu, Z, Xia, L, Xiao, J, Xu, L, Yang, Y, Yin, W, Yu, J, Yuan, L, Zhang, T, Zhang, L, Zhang, Y, Zhang, X, Zhu, L, Alfaro, A, Abrihan, P, Barroso, A, Cruz, E, Gomez, M, Magboo, V, Medina, J, Obaldo, J, Pastrana, D, Pawhay, C, Quinon, A, Tang, J, Tecson, B, Uson, K, Uy, M, Kostkiewicz, M, Kunikowska, J, Bettencourt, N, Cantinho, G, Ferreira, A, Syed, G, Arnous, S, Atyani, S, Byrne, A, Gleeson, T, Kerins, D, Meehan, C, Murphy, D, Murphy, M, Murray, J, O'Brien, J, Bang, J, Bom, H, Cho, S, Hong, C, Jang, S, Jeong, Y, Kang, W, Kim, J, Namgung, C, So, Y, Won, K, Majstorov, V, Vavlukis, M, Salobir, B, Stalc, M, Benedek, T, Benedek, I, Mititelu, R, Stan, C, Dariy, O, Drozdova, O, Gagarina, N, Gulyaev, V, Itskovich, I, Karalkin, A, Kokov, A, Migunova, E, Pospelov, V, Ryzhkova, D, Saifullina, G, Sazonova, S, Shurupova, I, Trifonova, T, Ussov, W, Vakhromeeva, M, Valiullina, N, Zavadovsky, K, Zhuravlev, K, Alasnag, M, Okarvi, S, Saranovic, D, Keng, F, See, J, Sekar, R, Yew, M, Vondrak, A, Bejai, S, Bennie, G, Bester, R, Engelbrecht, G, Evbuomwan, O, Gongxeka, H, Vuuren, M, Kaplan, M, Khushica, P, Lakhi, H, Louw, L, Malan, N, Milos, K, Modiselle, M, More, S, Naidoo, M, Scholtz, L, Vangu, M, Aguade-Bruix, S, Blanco, I, Cabrera, A, Camarero, A, Casans-Tormo, I, Cuellar-Calabria, H, Flotats, A, Canamero, M, Garcia, M, Leta, R, Diaz, J, Lumbreras, L, Marquez-Cabeza, J, Martin, F, De Alegria, A, Medina, F, Canal, M, Peiro, V, Pubul-Nunez, V, Madrid, J, Rey, C, Perez, R, Ruiz, J, Hernandez, G, Sevilla, A, Zeidan, N, Nanayakkara, D, Udugama, C, Simonsson, M, Alkadhi, H, Burger, P, Ceriani, L, De Boeck, B, Grani, C, De Saint Lager Lucas, A, Kamani, C, Kawel-Boehm, N, Manka, R, Prior, J, Rominger, A, Vallee, J, Khiewvan, B, Premprabha, T, Thientunyakit, T, Sellem, A, Kir, K, Sayman, H, Sebikali, M, Muyinda, Z, Kmetyuk, Y, Korol, P, Mykhalchenko, O, Pliatsek, V, Satyr, M, Albalooshi, B, Anderson, J, Bedi, P, Biggans, T, Bularga, A, Bull, R, Burgul, R, Carpenter, J, Coles, D, Cusack, D, Deshpande, A, Dougan, J, Fairbairn, T, Farrugia, A, Gopalan, D, Gummow, A, Ramkumar, P, Hamilton, M, Harbinson, M, Hartley, T, Hudson, B, Joshi, N, Kay, M, Kelion, A, Khokhar, A, Kitt, J, Low, C, Mak, S, Marousa, N, Martin, J, Mcalindon, E, Menezes, L, Morgan-Hughes, G, Moss, A, Murray, A, Patel, D, Peebles, C, Pugliese, F, Rodrigues, J, Rofe, C, Sabharwal, N, Schofield, R, Semple, T, Sharma, N, Strouhal, P, Subedi, D, Topping, W, Tweed, K, Weir-Mccall, J, Abbara, S, Abbasi, T, Abbott, B, Abohashem, S, Abramson, S, Al-Abboud, T, Al-Mallah, M, Almousalli, O, Ananthasubramaniam, K, Kumar, M, Askew, J, Attanasio, L, Balmer-Swain, M, Bayer, R, Bernheim, A, Bhatti, S, Bieging, E, Blankstein, R, Bloom, S, Blue, S, Bluemke, D, Borges, A, Branch, K, Bravo, P, Brothers, J, Budoff, M, Bullock-Palmer, R, Burandt, A, Burke, F, Bush, K, Candela, C, Capasso, E, Cavalcante, J, Chang, D, Chatterjee, S, Chatzizisis, Y, Cheezum, M, Chen, T, Chen, J, Chen, M, Choi, A, Clarcq, J, Cordero, A, Crim, M, Danciu, S, Decter, B, Dhruva, N, Doherty, N, Doukky, R, Dunbar, A, Duvall, W, Edwards, R, Esquitin, K, Farah, H, Fentanes, E, Ferencik, M, Fisher, D, Fitzpatrick, D, Foster, C, Fuisz, T, Gannon, M, Gastner, L, Gerson, M, Ghoshhajra, B, Goldberg, A, Goldner, B, Gonzalez, J, Gore, R, Gracia-Lopez, S, Hage, F, Haider, A, Haider, S, Hamirani, Y, Hassen, K, Hatfield, M, Hawkins, C, Hawthorne, K, Heath, N, Hendel, R, Hernandez, P, Hill, G, Horgan, S, Huffman, J, Hurwitz, L, Iskandrian, A, Janardhanan, R, Jellis, C, Jerome, S, Kalra, D, Kaviratne, S, Kay, F, Kelly, F, Khalique, O, Kinkhabwala, M, Iii, G, Kircher, J, Kirkbride, R, Kontos, M, Kottam, A, Krepp, J, Layer, J, Lee, S, Leppo, J, Lesser, J, Leung, S, Lewin, H, Litmanovich, D, Liu, Y, Lopez-Mattei, J, Magurany, K, Markowitz, J, Marn, A, Matis, S, Mckenna, M, Mcrae, T, Mendoza, F, Merhige, M, Min, D, Moffitt, C, Moncher, K, Moore, W, Morayati, S, Morris, M, Mossa-Basha, M, Mrsic, Z, Murthy, V, Nagpal, P, Napier, K, Narula, J, Nelson, K, Nijjar, P, Osman, M, Parwani, P, Passen, E, Patel, A, Patil, P, Paul, R, Phillips, L, Polsani, V, Poludasu, R, Pomerantz, B, Porter, T, Prentice, R, Pursnani, A, Rabbat, M, Ramamurti, S, Rich, F, Luna, H, Robinson, A, Robles, K, Rodriguez, C, Rorie, M, Rumberger, J, Russell, R, Sabra, P, Sadler, D, Schemmer, M, Schoepf, U, Shah, S, Shah, N, Shanbhag, S, Sharma, G, Shayani, S, Shirani, J, Shivaram, P, Sigman, S, Simon, M, Slim, A, Smith, D, Smith, A, Soman, P, Srichai-Parsia, M, Streeter, J, Albert, T, Tawakol, A, Thomas, D, Thompson, R, Torbet, T, Trinidad, D, Ullery, S, Unzek, S, Uretsky, S, Vallurupalli, S, Verma, V, Waller, A, Wang, E, Ward, P, Weissman, G, Wesbey, G, White, K, Winchester, D, Wolinsky, D, Yost, S, Zgaljardic, M, Alonso, O, Beretta, M, Ferrando, R, Kapitan, M, Mut, F, Djuraev, O, Rozikhodjaeva, G, Ngoc, H, Mai, S, Nguyen, X, Basic and Translational Research and Imaging Methodology Development in Groningen (BRIDGE), Translational Immunology Groningen (TRIGR), and Cardiovascular Centre (CVC)
Subjects: INCAPS COVID Investigators Group, cardiac imaging techniques, Settore MED/11 - Malattie dell'Apparato Cardiovascolare, Practice Patterns, Disease, Cardiovascular, coronary artery disease, COVID-19, Cardiac Imaging Techniques, Cardiologists, Europe, Health Care Surveys, Healthcare Disparities, Heart Diseases, Humans, Practice Patterns, Physicians', Predictive Value of Tests, Gross domestic product, Human health, cardiovascular disease, Pandemic, Medicine, cardiovascular imaging, BIOMEDICINA I ZDRAVSTVO. Kliničke medicinske znanosti. Interna medicina, cardiac imaging technique, Predictive value of tests, Cardiology and Cardiovascular Medicine, BIOMEDICINA I ZDRAVSTVO. Kliničke medicinske znanosti. Infektologija, cardiac disease, Coronavirus disease 2019 (COVID-19), Independent predictor, cardiac imaging, NO, Imaging diagnosis, Diseases of the circulatory (Cardiovascular) system, BIOMEDICINE AND HEALTHCARE. Clinical Medical Sciences. Internal Medicine, Physicians', business.industry, BIOMEDICINE AND HEALTHCARE. Clinical Medical Sciences. Infectology, RC666-701, HOSPITALIZATIONS, business, Health Care Delivery, Economics and Global Health Care, Demography
Abstract: ObjectivesWe aimed to explore the impact of the COVID-19 pandemic on cardiac diagnostic testing and practice and to assess its impact in different regions in Europe.MethodsThe online survey organised by the International Atomic Energy Agency Division of Human Health collected information on changes in cardiac imaging procedural volumes between March 2019 and March/April 2020. Data were collected from 909 centres in 108 countries.ResultsCentres in Northern and Southern Europe were more likely to cancel all outpatient activities compared with Western and Eastern Europe. There was a greater reduction in total procedure volumes in Europe compared with the rest of the world in March 2020 (45% vs 41%, p=0.003), with a more marked reduction in Southern Europe (58%), but by April 2020 this was similar in Europe and the rest of the world (69% vs 63%, p=0.261). Regional variations were apparent between imaging modalities, but the largest reductions were in Southern Europe for nearly all modalities. In March 2020, location in Southern Europe was the only independent predictor of the reduction in procedure volume. However, in April 2020, lower gross domestic product and higher COVID-19 deaths were the only independent predictors.ConclusionThe first wave of the COVID-19 pandemic had a significant impact on care of patients with cardiac disease, with substantial regional variations in Europe. This has potential long-term implications for patients and plans are required to enable the diagnosis of non-COVID-19 conditions during the ongoing pandemic.
Published: 2021

39. Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios

Author: Sánchez, C., Prat, J., Zacharegkas, G., Pandey, S., Baxter, E., Bernstein, G. M., Blazek, J., Cawthon, R., Chang, C., Krause, E., Lemos, P., Park, Y., Raveri, M., Sanchez, J., Troxel, M. A., Amon, A., Fang, X., Friedrich, O., Gruen, D., Porredon, A., Secco, L. F., Samuroff, S., Alarcon, A., Alves, O., Andrade-Oliveira, F., Bechtol, K., Becker, M. R., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Chen, R., Choi, A., Crocce, M., Davis, C., De Vicente, J., Derose, J., Di Valentino, E., Diehl, H. T., Dodelson, S., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Elvin-Poole, J., Everett, S., Ferté, A., Fosalba, P., Gatti, M., Giannini, G., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Huff, E. M., Huterer, D., Jarvis, M., Jain, B., Kuropatkin, N., Leget, P. -F., Maccrann, N., Mccullough, J., Muir, J., Myles, J., Navarro-Alsina, A., Rollins, R. P., Roodman, A., Rosenfeld, R., Rykoff, E. S., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troja, A., Tutusaus, I., Varga, T. N., Wechsler, R. H., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Bacon, D., Bertin, E., Bhargava, S., Brooks, D., Buckley-Geer, E., Burke, D. L., Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Desai, S., Dietrich, J. P., Doel, P., Evrard, A. E., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Kuehn, K., Lahav, O., Lima, M., Lin, H., Maia, M. A. G., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Palmese, A., Paz-Chinchón, F., Petravick, D., Pieres, A., Plazas Malagón, A. A., Rodriguez-Monroy, M., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Des, Collaboration, Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), DES, National Science Foundation (US), Department of Energy (US), Ministerio de Economía y Competitividad (España), European Research Council, Generalitat de Catalunya, European Commission, A Sánchez, C., Prat, J., Zacharegkas, G., Pandey, S., Baxter, E., Bernstein, G. M., Blazek, J., Cawthon, R., Chang, C., Krause, E., Lemos, P., Park, Y., Raveri, M., Sanchez, J., Troxel, M. A., Amon, A., Fang, X., Friedrich, O., Gruen, D., Porredon, A., Secco, L. F., Samuroff, S., Alarcon, A., Alves, O., Andrade-Oliveira, F., Bechtol, K., Becker, M. R., Camacho, H., Campos, A., Carnero Rosell, A., Carrasco Kind, M., Chen, R., Choi, A., Crocce, M., Davis, C., De Vicente, J., Derose, J., Di Valentino, E., Diehl, H. T., Dodelson, S., Doux, C., Drlica-Wagner, A., Eckert, K., Eifler, T. F., Elsner, F., Elvin-Poole, J., Everett, S., Ferté, A., Fosalba, P., Gatti, M., Giannini, G., Gruendl, R. A., Harrison, I., Hartley, W. G., Herner, K., Huff, E. M., Huterer, D., Jarvis, M., Jain, B., Kuropatkin, N., Leget, P. -F., Maccrann, N., Mccullough, J., Muir, J., Myles, J., Navarro-Alsina, A., Rollins, R. P., Roodman, A., Rosenfeld, R., Rykoff, E. S., Sevilla-Noarbe, I., Sheldon, E., Shin, T., Troja, A., Tutusaus, I., Varga, T. N., Wechsler, R. H., Yanny, B., Yin, B., Zhang, Y., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Bacon, D., Bertin, E., Bhargava, S., Brooks, D., Buckley- Geer, E., Burke, D. L., Carretero, J., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Desai, S., Dietrich, J. P., Doel, P., Evrard, A. E., Ferrero, I., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Kuehn, K., Lahav, O., Lima, M., Lin, H., Maia, M. A. G., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Palmese, A., Paz-Chinchón, F., Petravick, D., Pieres, A., Plazas Malagón, A. A., Rodriguez-Monroy, M., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., and UAM. Departamento de Física Teórica
Subjects: Gravitational Lensing, mice, Cosmology and Nongalactic Astrophysics (astro-ph.CO), challenge lightcone simulation, halo, Física, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, calibration, Astrophysics, Dark Energy, Astrophysic, Cosmology and Nongalactic Astrophysics, statistics, galaxies, luminosity, Weak, baryonic feedback, constraints, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], intrinsic alignments, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: C. Sánchez et al., Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale galaxy-galaxy lensing measurements around the same lens sample to constrain source redshift uncertainties, intrinsic alignments and other systematics or nuisance parameters of our model. Instead of using a simple geometric approach for the ratios as has been done in the past, we use the full modeling of the galaxy-galaxy lensing measurements, including the corresponding integration over the power spectrum and the contributions from intrinsic alignments and lens magnification. We perform extensive testing of the small-scale shear-ratio (SR) modeling by studying the impact of different effects such as the inclusion of baryonic physics, nonlinear biasing, halo occupation distribution descriptions and lens magnification, among others, and using realistic N-body simulations of the DES data. We validate the robustness of our constraints in the data by using two independent lens samples with different galaxy properties, and by deriving constraints using the corresponding large-scale ratios for which the modeling is simpler. The results applied to the DES Y3 data demonstrate how the ratios provide significant improvements in constraining power for several nuisance parameters in our model, especially on source redshift calibration and intrinsic alignments. For source redshifts, SR improves the constraints from the prior by up to 38% in some redshift bins. Such improvements, and especially the constraints it provides on intrinsic alignments, translate to tighter cosmological constraints when shear ratios are combined with cosmic shear and other 2pt functions. In particular, for the DES Y3 data, SR improves S8 constraints from cosmic shear by up to 31%, and for the full combination of probes (3×2pt) by up to 10%. The shear ratios presented in this work are used as an additional likelihood for cosmic shear, 2×2pt and the full 3×2pt in the fiducial DES Y3 cosmological analysis., C. S. is supported by Grant No. AST-1615555 from the U.S. National Science Foundation, and Grant No. DESC0007901 from the U.S. Department of Energy (DOE). J. P. is supported by DOE Grant No. DE-SC0021429. Funding for the DES Projects has been provided by the U.S. Department of Energy, the U.S. National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at UrbanaChampaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministerio da Ciência, Tecnologia e Inovação, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the Dark Energy Survey. The Collaborating institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energeticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DESBrazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ci`encies de l’Espai (IEEC/CSIC), the Institut de Física d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, The Ohio State UniverFIG. 16. Correlation matrix for the lensing ratios, on the left panel using the REDMAGIC lens sample and on the right panel using the MAGLIM sample. sity, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. The DES data management system is supported by the National Science Foundation under Grants No. AST1138766 and No. AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under Grants No. AYA2015-71825, No. ESP2015-88861, No. FPA2015-68048, No. SEV2012-0234, No. SEV-2016-0597, and No. MDM-20150509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC Grants Agreement No. 240672, No. 291329, and No. 306478.
Published: 2021
Full Text: View/download PDF

40. The mass and galaxy distribution around SZ-selected clusters

Author: Shin, T, Jain, B, Adhikari, S, Baxter, EJ, Chang, C, Pandey, S, Salcedo, A, Weinberg, DH, Amsellem, A, Battaglia, N, Belyakov, M, Dacunha, T, Goldstein, S, Kravtsov, AV, Varga, TN, Abbott, TMC, Aguena, M, Alarcon, A, Allam, S, Amon, A, Andrade-Oliveira, F, Annis, J, Bacon, D, Bechtol, K, Becker, MR, Bernstein, GM, Bertin, E, Bocquet, S, Bond, JR, Brooks, D, Buckley-Geer, E, Burke, DL, Campos, A, Rosell, A Carnero, Kind, M Carrasco, Carretero, J, Chen, R, Choi, A, Costanzi, M, da Costa, LN, DeRose, J, Desai, S, De Vicente, J, Devlin, MJ, Diehl, HT, Dietrich, JP, Dodelson, S, Doel, P, Doux, C, Drlica-Wagner, A, Eckert, K, Elvin-Poole, J, Everett, S, Ferraro, S, Ferrero, I, Ferté, A, Flaugher, B, Frieman, J, Gallardo, PA, Gatti, M, Gaztanaga, E, Gerdes, DW, Gruen, D, Gruendl, RA, Gutierrez, G, Harrison, I, Hartley, WG, Hill, JC, Hilton, M, Hinton, SR, Hollowood, DL, Hughes, JP, James, DJ, Jarvis, M, Jeltema, T, Koopman, BJ, Krause, E, Kuehn, K, Kuropatkin, N, Lahav, O, Lima, M, Lokken, M, MacCrann, N, Madhavacheril, MS, Maia, MAG, McCullough, J, McMahon, J, Melchior, P, Menanteau, F, Miquel, R, Mohr, JJ, Moodley, K, Morgan, R, Myles, J, Nati, F, Navarro-Alsina, A, Niemack, MD, Ogando, RLC, Page, LA, and Palmese, A
Subjects: clusters: general [galaxies], Astronomy & Astrophysics, evolution [galaxies], observations [cosmology], Astronomical and Space Sciences
Abstract: We present measurements of the radial profiles of the mass and galaxy number density around Sunyaev–Zel’dovich (SZ)-selected clusters using both weak lensing and galaxy counts. The clusters are selected from the Atacama Cosmology Telescope Data Release 5 and the galaxies from the Dark Energy Survey Year 3 data set. With signal-to-noise ratio of 62 (45) for galaxy (weak lensing) profiles over scales of about 0.2–20 h-1 Mpc, these are the highest precision measurements for SZ-selected clusters to date. Because SZ selection closely approximates mass selection, these measurements enable several tests of theoretical models of the mass and light distribution around clusters. Our main findings are: (1) The splashback feature is detected at a consistent location in both the mass and galaxy profiles and its location is consistent with predictions of cold dark matter N-body simulations. (2) The full mass profile is also consistent with the simulations. (3) The shapes of the galaxy and lensing profiles are remarkably similar for our sample over the entire range of scales, from well inside the cluster halo to the quasilinear regime. We measure the dependence of the profile shapes on the galaxy sample, redshift, and cluster mass. We extend the Diemer & Kravtsov model for the cluster profiles to the linear regime using perturbation theory and show that it provides a good match to the measured profiles. We also compare the measured profiles to predictions of the standard halo model and simulations that include hydrodynamics. Applications of these results to cluster mass estimation, cosmology, and astrophysics are discussed.
Published: 2021

41. Evaluation of appendicitis risk prediction models in adults with suspected appendicitis

Author: Nepogodiev, D., Matthews, J. H., Morley, G. L., Naumann, D. N., Ball, A., Chauhan, P., Bhanderi, S., Mohamed, I., Glasbey, J. C., Wilkin, R. J. W., Drake, T. M., Clements, J., Blencowe, N. S., Herrod, P. J. J., Pata, F., Frasson, M., Blanco-Colino, R., Soares, A. S., Nepogodiev D, Bhangu A., Matthews, Jh, Morley, Gl, Naumann, Dn, Ball, A, Chauhan, P, Bhanderi, S, Mohamed, I, Glasbey, Jc, Wilkin, R, Drake, Tm, Clements, J, Blencowe, Ns, Herrod, P, Pata, F, Frasson, M, Blanco-Colino, R, Soares, As, Bhangu, A, Nepogodiev, D, Jain, S, Amuthalingam, T, Tyler, R, Griffiths, Ea, Pinkney, Td, Gee, O, Morton, Dg, Beggs, A, Beral, D, Bowley, D, Cruickshank, N, Daniels, I, Griffiths, E, Hornby, St, Lund, Jn, Marriott, P, Singh, P, Smart, Nj, Speake, D, Thompson, C, Torkington, J, Torrance, A, Vohra, R, Warren, O, Winter, Dc, Pellino, G, Sgrò, A, Simioni, A, Farina, V, Podda, M, Di Saverio, S, Birindelli, A, Pasquali, S, Itsurg, Surg, Pt, Bolton, W, Bradshaw, Cj, Chean, Cs, Harris, G, Haddow, Jb, Jamieson, Nb, Mccain, S, Mason, J, Milgrom, D, Nana, Gr, Mohamed, Mn, Brien, Jo, Pearce, J, Rabie, M, Sahnan, K, Sarmah, P, Skerritt, C, Ghazanfar, Ma, Sreedharan, L, Kabwama, S, Gray, Rt, Kamande, Iw, Nazarian, S, Dar, Fa, Misky, At, Arunachalam, S, Twum-Barima, Cs, Mohamed, Im, Connor, Kl, Coe, Po, Kosti, A, Elshaer, M, Colvin, Da, Charalambous, Mp, Yeung, K, Merker, L, Morrison, T, Thaventhiran, Aj, Gilbert, Tm, Clements, Jm, Hicks, G, Afshar, S, Mckinley, Nc, Assaf, N, Hanna, T, Macinnes, E, Thavanesan, N, Dubois, As, Palani-Velu, Lk, Tezas, S, Yow, L, Radwan, Rw, Abdelrahman, M, Lee, Ka, Zarka, Za, Mcdowall, Na, Tan, Cy, Venn, Ml, Ashmore, Dl, Whitehorn, Se, Golder, Am, Reddy, A, Delimpalta, C, Kay, Oh, Shah, Sm, Eiben, I, Doyle, C, Tudyka, V, Issa, E, West, H, Brewer, Hk, Farrow, Ez, Taylor, Ns, Smart, Cj, Griffiths, Np, Halkias, C, Vitish-Sharma, P, Knight, Sr, Mowbray, Ng, Olivier, Jb, Lee, Kj, Clement, Kd, Chrastek, D, Panda, N, Connor, Mj, Fahmy, Se, Bryan, Es, Ngu, Ws, Adegbola, So, Vaughan, Em, Stupalkowska, W, Simmonds, L, Malik, A, Hussein, A, Karim, Mj, Singhal, T, Ormiston, R, Kung, V, Rabie, Ma, Park, Jh, Lal, N, Worku, D, D'Auria, M, Ang, A, Orizu, M, Gammeri, E, Clough, E, Choy, Ch, Lawday, S, Hann, Aj, Robinson, D, Wardle, Bg, Mcdonnell, D, Rutherford, Dg, Hickey, Lm, Garg, Ag, Rezvani, S, Bell, Cr, Mahmood, F, Rehman, S, Donaldson, G, Peleki, A, Pearce, L, Sharp, Ol, Singh, S, Thompson, Db, El-Tayar, O, Hollyman, M, Rupasinghe, Sn, Toomey, Db, Murray, Mp, Amtul, N, Mersh, Rj, Newton, Rc, Al-Khyatt, W, Stephens, Gf, Abbas, Sh, Iqbal, Mr, Brown, Ce, Renshaw, S, Hureibi, Ka, Pullabatla-Venkata, Up, Donohoe, No, Myatt, A, Egan, Rj, Rangarajan, K, Trail, M, Mckay, Sc, Engall, N, Jerome, E, Townsend, Dc, Patel, By, Pronin, S, Chandratreya, N, Choong, Jh, Mohamed, Tm, Hudson-Peacock, Nj, Manson, R, Hebbar, K, Mothe, Bs, Weegenaar, Cr, Saad, M, Bowman, Cr, Serventi, F, Fleres, F, Foppa, C, Pata, G, Baronio, G, Pertile, D, Lucchi, A, Sagnotta, A, Maretto, I, Campagnaro, T, Gatti, M, Gjoni, E, Roscio, F, Inama, M, Coccolini, F, Colombo, F, Avanzolini, A, Aresu, S, De-Manzoni-Garberini, A, Merlini, Da, Chessa, A, Tamini, N, Mulas, S, Cillara, N, Coletta, D, Atzeni, J, Erdas, E, Gallo, G, Francone, E, Di Gioia, P, Bianchi, Cl, Ferrara, F, Biancafarina, A, Scabini, S, Marano, L, Miegge, A, Sasia, D, Savino, G, Scatizzi, M, D'Amico, Fe, Arcuri, Ga, Gavagna, L, Salamone, G, Tatulli, F, Goldin, E, Matos, Ml, Caldeira, Ab, Romano, J, Pereira, J, Azevedo, J, Azevedo, Jm, Simoes, J, Silva, A, O'Leary, Dp, Kennedy, Nd, Quinn, Em, Zhang, Ay, Neary, Pm, De-Marchi, Ja, O'Connor, Br, Wijesundera, K, Foley, Nm, Wong, J, Tiedt, La, Bolger, Jc, Connelly, Tm, Ahmed, Os, Vigorita, V, García, V, Arredondo, J, Redondo, E, Sainz, B, Aldrey, I, Landaluce-Olavarria, A, Gómez, Aa, Cordoba, E, Sánchez-Fuentes, Mn, Cerdán-Santacruz, C, Beltran-De-Heredia, J, García, M, Veres, T, García-Novoa, A, Abellán, Am, García-Catalá, L, Ruiz-Marín, M, Menendez, P, Roldán-Ortiz, S, Navas-Cuéllar, Ja, Sabia, D, Gomez-Rosado, Jc, Navidad, Ms, Caula, C, Sanchez, Er, Espin-Basany, E, Fernández-Martínez, D, Bravo-Gutiérrez, Af, Payá-Llorente, C, Dujovne, P, Lima, F, Soria-Aledo, V, Gomez, Cj, Pascual-Miguelañez, I, Muinelo, M, Alvarez, Cm, Vargas-Pierola, Hj, Vallve-Bernal, M, Hidalgo-Rosas, Jm, Arenal-Vera, Jj, Sena-Ruiz, F, Sanchez-Guillen, L, Villarejo-Campos, P, Tallon-Aguilar, L, Garcea, A, Bennett, Jm, Whittaker, L, Gidwani, Al, Byrnes, Ck, Saunders, S, Shiwani, Mh, Ashraf, N, Venkatasubramaniam, Ak, Bevan, Ke, Mcarthur, D, Mustafa, Ak, Griffith, Jp, Blazeby, Jm, Charalabopoulos, A, Campbell, W, Reese, G, Warren, Oj, Peacock, M, Menzies, D, Jenner, D, Eardley, Nj, Yoong, S, Abulafi, M, Avalapati, H, Thompson, R, Nastro, P, Kochupapy, R, Stubbs, Bm, Mcintyre, R, Crozier, J, Patel, Pk, Pento, V, Beasley, Wd, Roxburgh, C, Youssef, H, Alexander, R, Denley, S, Di Franco, F, Quddus, A, Saha, A, Hunter, I, Hannay, J, Velchuru, Vr, Bond-Smith, G, Salama, Y, Bhargava, A, Panagiotopoulos, Sp, Watson, N, Garcea, G, Boddy, Ap, Dunning, Pg, Lloyd, G, Gurjar, Sv, Hill, J, Andrews, B, Singh, A, Ruzvidzo, F, Shingler, G, Mahon, D, Elgaddal, S, Payne, Cj, Shaikh, Ia, Dalmia, S, Nair, Ms, Finch, Jg, Chapple, Ks, Bawa, S, Watfah, J, Carden, Ca, Makhija, R, Rao, M, Sarveswaran, J, Vijay, V, Rekhraj, S, Knight, B, Siddiqui, Mn, Sebastian, Jf, Glen, P, Vakis, S, Ebied, H, Rajaram, R, Gray, J, Mcgrath, D, Faulkner, G, Gopalswamy, S, Varcada, M, Woodward, A, Williams, Gl, Szentpali, K, Ravindran, R, Bronder, C, Thaha, Ma, Rate, A, Shetty, Vd, Rao, V, Sajid, Ms, Clements, B, Patel, Rt, Mason, C, Branagan, G, Maude, K, Kaur, G, Lyons, A, Ainsworth, P, Hagger, R, Zadi, Az, Maslekar, Su, Kinross, J, Irukulla, S, Hawkins, W, Wheatstone, S, Magro, T, Bailey, S, Marshall, G, Mccullough, J, Marangoni, G, Leung, El, Borg, Cm, Gopinath, S, Kirkby-Bott, J, Yalamarthi, S, Mirza, S, Brett, M, Ramcharan, S, Pandey, V, Thava, B, Andreani, Sm, Sahay, Sj, Aravind, B, Downey, M, Nicol, D, Whitehouse, P, Sharma, A, Francis, N, Chitsabesan, P, Stewart, Dj, Norcia, Gg, Cucinotta, E, Cianchi, F, Romario, Uf, Taglietti, L, Capelli, P, Garulli, G, Parisi, A, Nitti, D, Guglielmi, A, Alonzo, A, Scandroglio, Is, Moretto, G, Ansaloni, L, Pietrabissa, A, Foschi, D, Vettoretto, N, Ercolani, G, Coppola, M, Colangelo, E, Morandi, E, Niolu, P, Pala, M, Coletti, M, Pisanu, A, Nicolosi, A, Sammarco, G, Berti, S, Soliani, P, Tonini, V, Stella, M, Ceccarelli, G, De Nisco, C, Castagnoli, G, De Nardi, P, Borghi, F, Agresta, F, Benevento, A, Cantafio, S, Cesari, Mc, Rubbini, M, Chetta, G, De Marchi, F, Nora, Mf, Sousa, Hs, Nascimento, Ca, Casimiro, C, Costa, Sd, Rosa, Mj, Carvalho, N, Correia, J, Gomes, Ap, Hill, Ad, Walsh, Tn, Aremu, Ma, Mulsow, J, El-Masry, S, Gillick, J, Garvin, J, Caldwell, M, Mehigan, B, Peirce, Cb, Cooke, F, Mealy, K, Ruano, A, Ais, G, Fueyo, J, Parajó, Ae, Bernal-Sprekelsen, Jc, Monzón-Abad, Ja, Blanco, F, Arroyo, A, Bazán-Hinojo, Mc, Ramos-Bernado, Mi, Lopez-Ruiz, Ja, Golda, T, Julià, D, Cuadrado, Mm, Gómez-Abril, Sa, Martinez, J, Aguayo, Jl, Millan, M, Alvarez-Gallego, M, Muinelo-Lorenzo, M, Parra, Jm, Muñoz-Muñoz, E, De Chaves-Rodríguez PG, Cánovas-Moreno, G, Rodriguez-Lopez, M, Segura-Sampedro, Jj, García-Granero, A, Redondo-Calvo, Fj, Dyson, S, Thakur, D, Swords, C, Siaw, O, Zelazek, M, Woo, R, Badran, A, Aruparayil, N, Christopoulos, P, Chambers, B, O'Neill, N, Long, Rh, Mccaughey, P, Wong, Ml, Mccain, Rs, Lennox-Warburton, Hc, Moore, C, Manektella, Km, Mcilwaine, S, Rupani, S, Simpson, Dj, Wauchope, J, Ng, M, Christian, L, Crone, A, Sacks, R, Symons, N, Lazzaro, A, Patil, Sd, Roomi, S, Silva, I, Hodgson, Jm, Ly, C, Froud, H, Patel, H, Cay, P, Karwal, Rs, Danquah-Boateng, D, Berry, B, Esmail, Hd, Maripi, H, Bilku, D, Mckelvie, Ma, Miller, K, Maina, A, Velho, R, Hasan, R, Clingan, R, Jah, S, Waite, K, Jones, A, Buckley-Jones, S, Lecky-Thompson, L, Saghir, N, Mansoor, S, Mistry, D, Brown, R, Wong, A, Gurung, S, Wensley, F, Fleming, Ta, Griggs, R, Haines, S, Bedoya, S, Beverstock, A, Johnson, J, Govind, G, Niaz, O, Dyal, A, Tokidis, E, Punj, S, Leusink, A, Rudland, I, Kelly, M, Morgan, R, Al-Musawi, S, Lek, C, Gilbert, A, Gosal, A, Mahoney, R, Parwaiz, I, Mitchard, Mj, Ribeiro, B, Merai, H, Dean, Ea, Khan, S, Baginski, A, Mann, C, Foers, W, Jones, L, Woodward, B, Mcwhirter, Dm, Thomas, At, Gilbert, Tg, Weatherburn, Lw, Pilkington, Jp, Cameron, Fc, Clements, Jd, Mccann, C, Davidson, S, Hackney, L, Clements, Js, Martin, A, Du, Dt, Shakoor, Z, Yen, Sk, Adnan, M, Ranathunga, S, Sana, S, Tay, Yh, Chin, My, Gillespie, M, Brown, Ag, Campbell, U, Chatzikonstantinou, M, Mahendran, B, Flack, T, Chowdhary, M, Lim, Jm, Whiteman, E, Shepherd, Ja, Pedder, A, Siggens, Kl, Lai, Cw, Morrison-Jones, V, Hayat, Z, Nehikhare, I, Macleod, C, Quinn, Hc, Brown, A, Neagle, G, Chok, Sm, Carrano, Fm, Abbassi, Oa, Divekar, Ga, Halmer, S, Adams, Re, Davies, Pl, Wong, Sy, Amarasinghe, R, Tague, Le, Jones, E, Singh, J, Boza, K, Kelly, Sd, Morrison, F, Chan, Wh, Wilson, Ej, Awokoya, Oo, Griffiths, Sn, Kirkham, En, Cotton, Ae, Adimonye, A, Leighton, Pa, Abdelrahman, A, Cartwright, H, Gates, Z, Miguras, M, Khan, K, Louw, C, Grove, T, Badenoch, T, Mckeon, J, Wood, Cs, Leitch, Rp, Sgardelis, P, Perera, Mi, Nagarajan, D, Malam, Y, Theodoropoulou, K, Rajagopal, S, Kaptanis, S, Popova, D, Olagbaiye, O, Tayeh, S, Rigby, S, Harris, Mp, Ren, Kz, Liaw, G, Zhou, S, White, F, Marshall, Cm, Mitchell, Jh, Anderson, Dj, Kanakala, V, Hollingsworth, A, Paramasevon, Kr, Milward, J, Ahmed, S, Fanibi, Bf, Ferguson, N, Dickson, Ea, Shaw, Av, Dixon, F, Morrish, S, Dandy, R, Fooks, P, Sharma, P, Islam, N, Tabain, V, Keegan, R, Ahel, J, Alhammali, T, Graveston, J, Balai, Ej, Rothnie, K, Pankin, Gp, Eiben, Ie, Jackson, Nj, Dhar, M, Nash, D, Dharamavaram, S, Seth, M, Chowdhury, F, Rezacova, M, Seneviratne, N, Turner, Ej, Currow, C, Isherwood, Jd, Hobson, Bm, Lui, Dh, Rodger, V, Ting, N, Photiou, D, Taze, D, Lodhia, S, Earnshaw, L, Kumar, K, Neale, A, Bastianpillai, J, Cipparrone, M, Barrie, A, Nash, Z, Anandan, L, Tailor, K, Vinnicombe, Z, Krivan, S, Kuo, R, Giorga, A, Habib, H, Malik, K, Bogdan, M, Mahon-Daly, Fp, Athersmith, Mj, Strange, Ja, Wheeler, C, Summerfield, L, Khaw, Ra, Ashour, O, Iosif, E, Fadel, M, Gopalakrishnan, K, Orme, N, Williams, S, Rashid, M, Sultana, A, Patel, N, Pearson, R, Yasin, T, Bevan, V, Al-Sarireh, B, Brown, M, Mohd, N, Howie, Ee, Poudevigne, M, Paget, C, Rallage, H, Chui, K, Fawzi, F, Layman, S, Okorocha, E, Jama, Gm, Orawiec, P, Kouli, O, Hassane, A, Kilkenny, J, Devine, Aa, Laurenson, M, Slezak, I, Barker, T, Lau, E, Limbada, M, O'Brien, J, Weaver, J, Hajibandeh, S, Shah, J, Mansour, Mm, Malik, Sn, Davis, S, Trew, F, Bandyopadhyay, Sk, Dart, K, Guru-Naidu, S, Callan, R, Nair, Mk, Alani, M, Sezen, E, Salim, S, Shurlock, J, Siddique, K, Forouzanfar, A, Brews, R, Acharya, A, Jain, A, Tozer, Pj, Warusavitarne, J, Emslie, Km, Collier-Wakefield, O, Sivaloganathan, P, Dobson, C, Elseedawy, M, Mcnally, L, Williams, M, Motiwala, Fh, Choi, S, Asmadi, Aa, Burnside, D, Everden, A, Suriyakumar, S, Sandu, L, Kent, Da, Bowen, J, Long, P, Khair, A, Shah, K, Phelan, L, Pierre, R, Dhari, Aa, Hoff, M, Nickson, S, Setshwaelo, T, Chalk, A, Parkola, Mj, Harlinska, A, Chan, T, Dudek, Jg, Rolph, R, Allen, M, Pollard, H, Gormely, R, Finlayson, H, Ljungqvist, G, Peponis, C, Rahman, M, Dhesi, S, Arshad, F, Faris, Ar, Sooriyamoorthy, T, Springate, El, Barnieh, W, Patel, As, Siddiqui, Za, Chishti, Ia, Ayube-Brown, J, Rabie, Mr, Blake, L, Yardimci, E, Nagendram, S, Neophytou, Gi, Henderson, L, Farhan-Alanie, M, Kong, Cy, Ghazala, R, Evans, J, Hussain, N, Kabir, M, Hraishawi, I, Cox, M, Bailey, Ja, Muhibullah, N, Yanni, F, Stevenson, R, Nair, A, Murphy, C, Mcgucken, O, Pandya, R, Bowerman, H, Lafaurie, G, Van Boxel GI, Shanmugarajah, K, Maragouthakis, D, Hanif, Z, Evans, Jd, Yoganathan, S, Richardson, Td, Cook, V, Clark, Gl, Rigney, B, O'Neill, E, Guliani, J, Chan, D, Harper, F, Sian, T, Boereboom, C, Blackwell, J, Hardy, E, Boyd-Carson, H, Couch, Dg, Barter, Ca, Thoukididou, Sn, Hatt, Jr, Jones, Cs, Dean, S, Rajaretnam, N, Masood, M, Thakral, N, Griffith, D, Doherty, C, Longshaw, A, Peprah, D, Mathew, G, Hook, A, Vance-Daniel, J, Ibrahim, Y, Walters, Kj, Whewell, He, Sherif, Ma, Mckenna, M, O'Sullivan, D, Woodrow, C, Gill, S, Johnstone, A, Gentry, R, Irwin, R, Forgie, A, Welsh, S, Ivey, P, Bullivant, Jk, English, Wj, Osterberg, A, Morowala, A, Al-Faham, Z, Islam, S, Tan, E, Sadek, S, Sihra, N, Shrestha, D, Chong, B, Nadeem, A, Fasuyi, Ja, Patel, Mm, Daureeawoo, R, Okekunle, B, Cheruvu, M, Mazumdar, E, Hussain, A, Patel, C, Mcquaid, M, Banks, A, Robinson, A, Khan, Ms, Riaz, W, Verroiotou, M, Cohen, Ja, Kouroumpas, E, Ghaffari, I, Moradzadeh, J, Kamal, M, Gulamhussein, M, Gaines, E, Ghatorae, S, Clark, S, Savill, A, Hutchinson, B, Chapman, J, Wu, F, Creasy, W, Raymond, M, Grosvenor, S, Odeh, A, Malik, Y, Bansal, H, Grant, C, Raofi, A, Ahmed, B, Mai, D, Souter, J, Hamelmann, Rn, Ikram, S, Durbacz, M, Gilliland, N, Salem, A, Chudek, D, Ladwa, N, Storey, R, Fontaine, C, Toomey, D, Miller, B, Oakey, M, Smoker, H, Chapman, Sj, O'Hagan, Sc, Tahir, W, Wilcox, G, Ahmad, A, Akram, F, Baddams, Ts, Boshier, Pr, Fehervari, M, Easdon, S, Ilozue, T, Adam, Me, Jokhan, S, Foster, A, Nambiar, K, Bohra, P, Janardanan, S, Shanmuganathan, V, Maqboul, F, Ettles, C, Wardle, Sd, Martinou, E, Khasria, A, Bagga, R, Motter, D, Mundkur, N, Pan, Y, Akbari, K, Farrell, Sm, Rahim, A, Gummaraju, A, Mahmoud, A, Akinsola, O, Smallcombe, N, Tarazi, M, Hanley, C, Campbell, Um, Franklin, D, Davidson, Jr, Raza, Ss, Krishnamoorthy, A, Rajjoub, Y, Ali, M, Seddon, Tc, Payne, Re, Das, A, Martin, Lm, Naismith, Kn, Venkata, Up, Manda, Vm, Burns, Km, Huang, J, Samuel, M, Docherty, Ja, Cheah, Wl, Ooi, R, Nyeko-Lacek, M, Marsh, L, Prideaux, A, Li, Ch, Poacher, A, Lee, M, Muzaffar, M, Kara, A, Walsh, E, Sunter, H, Roth, N, Roy, C, Mcmorran, D, Turnbull, A, Layton, Gr, Archer, Je, Yang, P, Douka, E, Amin, V, Borghol, K, Blackford, Od, Bond, S, Baker, B, Mohamed, Wo, Williams, R, Garnham, J, Robb, Hd, Allington, J, Cloney, L, Tamborska, A, Kalia, K, Fung, E, Johnston, Z, Lynch, L, Christides, A, Tan, Hl, Cynthia, G, Tsang, B, Rossi, C, Kaubrys, M, Al-Khafaji, N, Jenkins, M, Peiris, Gb, Gunning, S, Nimako, E, Pandya, D, Hever, P, Amayo, A, Bull, C, Clements, C, Al-Sheikh, M, Savioli, F, Long, M, Horsfield, E, Robertson, C, Ogboru, S, Mcilwrath, Ac, Bell, J, Limb, C, Obeid, N, Rich, Je, Balasubramaniam, A, Mashar, R, Taylor, M, Bruce, Js, Dennison, G, Curtis, Nj, Ezerska, E, Ellis, B, Wiggill, S, Tee, A, Ng, S, Carder, C, Abdelwahed, A, Chandler, Sb, Tinsley, Bj, Finotti, E, Occhioni, G, Cossu, F, Vulcano, I, Viscosi, F, Michelini, M, Compagnoni, B, Sepe, C, Isolani, Sm, Regina, G, Alagna, V, Martorelli, G, Gabbianelli, C, Moroni, P, Zuin, M, Conci, S, Lazzari, G, Costamagna, D, Zurleni, Tz, Altomare, Ma, Desiderio, J, Di Cintio, A, Gemini, A, Trastulli, S, Viviani, E, Tomasoni, M, Montori, G, Harder, G, Argenti, F, Malabarba, S, Checcacci, P, Montanelli, P, Guerra, F, Skalamera, I, Staderini, F, Grandi, S, Nelli, T, Coratti, F, Sorrentino, L, Maffioli, A, Cavallo, D, Bondurri, A, Groppo, G, Curti, R, Solaini, L, Xidas, A, Manias, T, Delogu, D, Vacca, A, Solinas, L, Corbellini, C, Fiore, L, Nigro, A, Santurro, L, Angrisani, M, Sparta, C, Lorettu, A, Mura, Fa, Ruggiu, Gv, Pirari, Pf, Pau, R, Melis, M, Piu, F, Patti, S, Deserra, A, Angelieri, D, Del Basso, C, Rossi, D, Iannone, I, De Padua, C, Giubilo, C, Falaschi, F, Cirillo, B, Gordini, L, Podda, F, Sanna, S, Saba, A, Poillucci, G, Pinna, E, Messina, A, Sena, G, Cardona, R, De Luca, E, Sacco, R, Vescio, G, Ammendola, M, Romano, R, Bianco, A, Bonfante, P, D'Ambra, L, Feleppa, C, Gennai, A, Lizzi, V, Moggia, E, Imperatore, M, Bolzon, S, Belvedere, A, Amaducci, E, Ripoli, Mc, Segalini, E, Cervellera, M, Vaccari, S, Eretta, Co, O'Neill, R, Llewelyn, O, Jones, N, Clerici, F, Ballabio, M, Andolfi, E, Angelini, M, Fontani, A, Miranda, E, Scricciolo, M, Provenza, G, Pellicanò, Ga, Pulighe, F, Argenio, G, Melis, A, Balestra, F, Anania, M, Cruccu, A, Massaiu, C, Murru, Ml, Martino, A, Luzzi, Ap, La Valle, G, Chillitupa, Cz, Bartoli, A, Conti, D, Spaziani, A, Bellochi, R, Listorti, C, Salandini, Mc, Carlucci, M, Tenconi, Sm, Cannavò, M, Marano, A, Giuffrida, Mc, Cannata, G, Pellegrino, L, Giraudo, G, Baraghini, M, Garzi, A, Giudicissi, R, Zalla, T, Romoli, L, Vannucchi, A, Giani, I, Feroci, F, Calussi, M, Ribaudo, M, Fiorot, A, Stecca, T, Nistri, C, Fornasier, C, Valiani, Sv, Brunelli, Db, Evoli, Le, Giuliani, Ng, Contine, Ac, Renzi, Cr, Feo, Cv, Anania, G, Carcoforo, P, Aisoni, F, Licari, L, Tutino, R, Cocorullo, G, Silvestri, V, De Marco, P, Fontana, T, Orlando, G, Falco, N, Baseggio, M, Napetti, S, Mella, A, Rossi, Gm, Chimetto, A, Cosci, M, Bonomo, M, Scialandrone, G, Chetta, N, Carvalho, Lc, Magalhães, Js, Pereira, Am, Fernandes, C, Fareleira, A, Gonçalves, D, Pais, M, Pereira, A, Resende, Fm, Correia, D, Cardoso, D, Tojal, A, Santos, Sc, Barbosa, L, Louro, Hc, Bairos, F, Martins, Fm, Messias, Fm, Ferreira, Ms, Borges, Fc, Botelho, P, Lima, M, Valente, Pm, João, Aa, Guimarães, Jm, Rocha, R, Nogueira, St, Kabir, U, Wong, C, Rahmani, Ls, Tan, S, Chng, S, Jasinski, B, Cheng, Sa, Mardhiah, S, Mcglynn, K, Hannan, E, Burke, J, Haveliwala, Z, O'Neill, M, Boland, M, Hayes, C, Fox, A, Zaborowski, A, Mitru, Rm, Mc-Dermott, A, Coyle, D, Stoica, I, Mcmahon, Sv, Laughlin, Dm, Kannegieser-Bailey, M, Murphy, R, Muntean, A, Shet, S, Thomas, L, De Freitas, S, Quill, S, Aljorfi, A, Soh, B, Law, Jj, Hartnett, J, Jansen, T, Gilgan, J, Jung, J, Scanlon, K, Szucs, A, Ahern, Dp, Redmond, Ae, Edwards, Se, Manoharan, P, Brennan, S, Abdelgadir, Am, Mckevitt, Kl, Zarog, Ma, Ahmed, G, Bukhari, W, Ahad, A, Paniagua, M, Samartin, C, Primo, Jc, Garrido, L, Lopez, M, Rufo, E, Trostchansky, I, Rodriguez, L, Infante, H, Acosta, A, Cremades, P, Cidoncha, A, Olmos, V, Oliva, I, Santamaria, C, Cavero, A, Calvo, H, Suero, Ca, Maderuelo, Vm, Galvez, P, Hernando, A, Eguaras, I, Recreo, Ac, García-Carrero, M, Moreda, R, De Andres, U, Del Pozo, E, Calvo, M, Moratalla, Cn, Ronda, Rn, Contreras, Rg, De Burgos CB, Cortés, Gv, Martínez, Cc, Agudo, Ar, Soriano, Jt, Ramos, Xh, Echazarreta, E, Elia, M, Hernaez, A, Sanchez, L, Vallejo-Bernad, C, Oliver, Jr, Sánchez-Rubio, M, Kälviäinen, Hk, Genzor, S, González-Nicolás, T, Puerta, E, Laviano, E, Gimenez, T, Fermiñán, A, Muriel-Álvarez, P, Sierra-Grañón, Je, Escoll-Rufino, J, Cuello-Guzmán, E, Mestres-Petit, N, Merichal-Resina, M, Pinillos-Somalo, A, Gomez-Carmona, Z, Vazquez-Fernandez, Ap, Trujillo-Diaz, Jj, Couso, Jr, Fernández, Md, Riera, E, Espinosa, J, Carral-Freire, M, Martínez-Almeida, R, Santarrufina-Martínez, S, Sebastián-Tomás, Jc, Gonzálvez-Guardiola, P, Fernández, Ec, Mozo, As, Stoyanov, Ti, Santamaría, Pc, Grimaldo, Eg, Fernández-Candela, A, Curtis-Martínez, C, Del-Valle-Ruiz, Sr, Sánchez-Cifuentes, A, Ramírez-Faraco, M, López, Af, Leon, C, Kumar, S, Fornell-Ariza, M, Ayllón-Gámez, S, Peña-Barturen, C, Ojea-Ruiz-Yherla, L, Saavedra-Chacón, M, Perez-Calvo, J, Gomez-Facundo, H, Riba-Combatti, L, Manas, Oc, De-Soto-Cardenal, B, De-La-Herranz-Guerrero, P, Dominguez-Sanchez, C, Gamero-Huaman, Jc, Suarez-Cabrera, A, Ramirez-Redondo, Aa, Lara-Fernandez, Y, Bascuas-Rodrigo, B, Lopez-Duran, Bl, Pigem, A, Gil, J, Salvador, H, Planellas, P, Farrés, R, Caballero, A, Arnau, M, Tapiolas, I, Ridaura, N, Roncero, Ls, Collado-Roura, F, Fijo, Lm, Cormenzana, Ob, Viñas, Nl, Grifell, Ms, Prats, Ma, Torrado, Aa, Sanz-Navarro, S, Contreras-Saiz, E, Solar-García, L, Moreno-Gijón, M, Suárez-Sánchez, A, Díaz-Vico, T, Rodicio-Miravalles, Jl, García-Gutierrez, C, Pila, U, Melone, S, Martin-Prieto, L, Rojo, Ja, Gonzalez, M, Zorrilla, L, Garcia-Marin, Ja, Baeza-Murcia, M, Pellicer-Franco, E, Jimenez-Ballester, Ma, Asensio-Gomez, L, Gortazar-De-Las-Casas, S, Guevara-Martinez, J, Ramirez, L, Verea, S, Anguita, F, Navarro, G, Criado, Adc, Lara, Mc, Martinez, Et, Sanchez-Martinez, A, Hernandez-Gimenez, L, Galofre-Recasens, M, Ferrer-Vilela, I, Pérez-Sanchez, Le, Esteves, Mb, Menéndez-Moreno, A, Baz-Figueroa, C, Rosat, A, Hontoria, Ms, García, Na, Gracia-Roman, R, Pascua-Sole, M, Pino-Perez, O, García-Pérez, Jm, Pineño-Flores, C, Ambrona-Zafra, D, Sancho-Muriel, J, Alvarez, E, Jiménez-Rosellón, R, Daga, O, Alberca-Paramo, A, Sanchez-Garcia, S, García-Santos, E, Pareja-Ciuró, F, Olivares-Oliver, C, Navarro-Morales, L, Tamayo-López, Mj, Tinoco-González, J, García-Rivera, Co, Agua, Ia, Moreno-Suero, F, Pereira-Mosquera, E, Zerpa, C, Llacer, E, Diaz, A, Caro, A, Feliu, F, Franco, M, Escuder, J, Abellan, M, Padilla, E, Mambrilla-Herrero, S, Plua-Muniz, Kt, Bailon-Cuadrado, M, Tejero-Pintor, Fj, Choolani-Bhojwani, E, Vila-Zarate, C, Delgado-Plasencia, Lj, Ponchietti, L, Cousins, L, Busuttil, A, Baird, C, Drye, N, Brown, Od, Mansour, S, Anderson, O, Mahapatra, R, Clements, Ja, D'Souza, N, Littlehales, Dj, Tang, Am, Byrne, Be, Cunha, P, Ogbuokiri, C, Eiben, P, Gravante, G, Kho, H, Dobbs, S, Doulias, T, Ng, J, Wilson, M, Venugopal, R, Wolff, J, Akhtar, K, Walji, Hd, Tognarelli, Jm, Knight, Ka, Ansari, A, Hussaini, Sa, Wright, E, Brewer, H, Rinkoff, S, Harries, Rl, Fairfield, Cj, Abbott, T, Jackson, A, Wright, Hl, Walters, U, Carney, K, Logan, Pc, Mughal, Z, Strachan, E, Chasty, B, Ma, J, Mazzeo, C, Badii, B, Armellini, A, Grassia, M, Perin, A, Ruzzenente, A, Magnoli, M, Depalma, N, Longheu, A, Papandrea, M, Dova, L, De Prizio, M, Gusai, Gp, Di Zitti, L, Geretto, P, Azabdaftari, A, Chianese, G, Elbetti, C, Ruffolo, C, Giaccari, S, Devezas, V, Ferreira, Js, Peixoto, R, Alshafei, A, Simo, V, José, Hs, Ugarte-Sierra, B, Salva, Ab, Gómez, N, Marinello, F, Medina-Arana, V, Vega, L, Ballester, Mm, Espina, B, Prieto-Nieto, Mi, Rodríguez, Ec, Padilla-Valverde, D, Duran-Muñoz-Cruzado, Vm., Nepogodiev, D, Matthews, Jh, Morley, Gl, Naumann, Dn, Ball, A, Chauhan, P, Bhanderi, S, Mohamed, I, Glasbey, Jc, Wilkin, R, Drake, Tm, Clements, J, Blencowe, N, Herrod, P, Pata, F, Frasson, M, Blanco-Colino, R, Soares, A, Bhangu, A, Jain, S, Amuthalingam, T, Tyler, R, Griffiths, Ea, Pinkney, Td, Gee, O, Morton, Dg, Beggs, A, Beral, D, Bowley, D, Cruickshank, N, Daniels, I, Griffiths, E, Hornby, St, Lund, Jn, Marriott, P, Singh, P, Smart, Nj, Speake, D, Thompson, C, Torkington, J, Torrance, A, Vohra, R, Warren, O, Winter, Dc, Pellino, G, Sgrò, A, Simioni, A, Farina, V, Podda, M, Di Saverio, S, Birindelli, A, Pasquali, S, Itsurg, Surg, Pt, Bolton, W, Bradshaw, Cj, Chean, C, Harris, G, Haddow, Jb, Jamieson, Nb, Mccain, S, Mason, J, Milgrom, D, Nana, Gr, Mohamed, Mn, Brien, Jo, Pearce, J, Rabie, M, Sahnan, K, Sarmah, P, Skerritt, C, Ghazanfar, Ma, Sreedharan, L, Kabwama, S, Gray, Rt, Kamande, Iw, Nazarian, S, Dar, Fa, Misky, At, Arunachalam, S, Twum-Barima, C, Mohamed, Im, Connor, Kl, Coe, Po, Kosti, A, Elshaer, M, Colvin, Da, Charalambous, Mp, Yeung, K, Merker, L, Morrison, T, Thaventhiran, Aj, Gilbert, Tm, Clements, Jm, Hicks, G, Afshar, S, Mckinley, Nc, Assaf, N, Hanna, T, Macinnes, E, Thavanesan, N, Dubois, A, Palani-Velu, Lk, Tezas, S, Yow, L, Radwan, Rw, Abdelrahman, M, Lee, Ka, Zarka, Za, Mcdowall, Na, Tan, Cy, Venn, Ml, Ashmore, Dl, Whitehorn, Se, Golder, Am, Reddy, A, Delimpalta, C, Kay, Oh, Shah, Sm, Eiben, I, Doyle, C, Tudyka, V, Issa, E, West, H, Brewer, Hk, Farrow, Ez, Taylor, N, Smart, Cj, Griffiths, Np, Halkias, C, Vitish-Sharma, P, Knight, Sr, Mowbray, Ng, Olivier, Jb, Lee, Kj, Clement, Kd, Chrastek, D, Panda, N, Connor, Mj, Fahmy, Se, Bryan, E, Ngu, W, Adegbola, So, Vaughan, Em, Stupalkowska, W, Simmonds, L, Malik, A, Hussein, A, Karim, Mj, Singhal, T, Ormiston, R, Kung, V, Rabie, Ma, Park, Jh, Lal, N, Worku, D, D'Auria, M, Ang, A, Orizu, M, Gammeri, E, Clough, E, Choy, Ch, Lawday, S, Hann, Aj, Robinson, D, Wardle, Bg, Mcdonnell, D, Rutherford, Dg, Hickey, Lm, Garg, Ag, Rezvani, S, Bell, Cr, Mahmood, F, Rehman, S, Donaldson, G, Peleki, A, Pearce, L, Sharp, Ol, Singh, S, Thompson, Db, El-Tayar, O, Hollyman, M, Rupasinghe, Sn, Toomey, Db, Murray, Mp, Amtul, N, Mersh, Rj, Newton, Rc, Al-Khyatt, W, Stephens, Gf, Abbas, Sh, Iqbal, Mr, Brown, Ce, Renshaw, S, Hureibi, Ka, Pullabatla-Venkata, Up, Donohoe, No, Myatt, A, Egan, Rj, Rangarajan, K, Trail, M, Mckay, Sc, Engall, N, Jerome, E, Townsend, Dc, Patel, By, Pronin, S, Chandratreya, N, Choong, Jh, Mohamed, Tm, Hudson-Peacock, Nj, Manson, R, Hebbar, K, Mothe, B, Weegenaar, Cr, Saad, M, Bowman, Cr, Serventi, F, Fleres, F, Foppa, C, Pata, G, Baronio, G, Pertile, D, Lucchi, A, Sagnotta, A, Maretto, I, Campagnaro, T, Gatti, M, Gjoni, E, Roscio, F, Inama, M, Coccolini, F, Colombo, F, Avanzolini, A, Aresu, S, De-Manzoni-Garberini, A, Merlini, Da, Chessa, A, Tamini, N, Mulas, S, Cillara, N, Coletta, D, Atzeni, J, Erdas, E, Gallo, G, Francone, E, Di Gioia, P, Bianchi, Cl, Ferrara, F, Biancafarina, A, Scabini, S, Marano, L, Miegge, A, Sasia, D, Savino, G, Scatizzi, M, D'Amico, Fe, Arcuri, Ga, Gavagna, L, Salamone, G, Tatulli, F, Goldin, E, Matos, Ml, Caldeira, Ab, Romano, J, Pereira, J, Azevedo, J, Azevedo, Jm, Simoes, J, Silva, A, O'Leary, Dp, Kennedy, Nd, Quinn, Em, Zhang, Ay, Neary, Pm, De-Marchi, Ja, O'Connor, Br, Wijesundera, K, Foley, Nm, Wong, J, Tiedt, La, Bolger, Jc, Connelly, Tm, Ahmed, O, Vigorita, V, García, V, Arredondo, J, Redondo, E, Sainz, B, Aldrey, I, Landaluce-Olavarria, A, Gómez, Aa, Cordoba, E, Sánchez-Fuentes, Mn, Cerdán-Santacruz, C, Beltran-De-Heredia, J, García, M, Veres, T, García-Novoa, A, Abellán, Am, García-Catalá, L, Ruiz-Marín, M, Menendez, P, Roldán-Ortiz, S, Navas-Cuéllar, Ja, Sabia, D, Gomez-Rosado, Jc, Navidad, M, Caula, C, Sanchez, Er, Espin-Basany, E, Fernández-Martínez, D, Bravo-Gutiérrez, Af, Payá-Llorente, C, Dujovne, P, Lima, F, Soria-Aledo, V, Gomez, Cj, Pascual-Miguelañez, I, Muinelo, M, Alvarez, Cm, Vargas-Pierola, Hj, Vallve-Bernal, M, Hidalgo-Rosas, Jm, Arenal-Vera, Jj, Sena-Ruiz, F, Sanchez-Guillen, L, Villarejo-Campos, P, Tallon-Aguilar, L, Garcea, A, Bennett, Jm, Whittaker, L, Gidwani, Al, Byrnes, Ck, Saunders, S, Shiwani, Mh, Ashraf, N, Venkatasubramaniam, Ak, Bevan, Ke, Mcarthur, D, Mustafa, Ak, Griffith, Jp, Blazeby, Jm, Charalabopoulos, A, Campbell, W, Reese, G, Warren, Oj, Peacock, M, Menzies, D, Jenner, D, Eardley, Nj, Yoong, S, Abulafi, M, Avalapati, H, Thompson, R, Nastro, P, Kochupapy, R, Stubbs, Bm, Mcintyre, R, Crozier, J, Patel, Pk, Pento, V, Beasley, Wd, Roxburgh, C, Youssef, H, Alexander, R, Denley, S, Di Franco, F, Quddus, A, Saha, A, Hunter, I, Hannay, J, Velchuru, Vr, Bond-Smith, G, Salama, Y, Bhargava, A, Panagiotopoulos, Sp, Watson, N, Garcea, G, Boddy, Ap, Dunning, Pg, Lloyd, G, Gurjar, Sv, Hill, J, Andrews, B, Singh, A, Ruzvidzo, F, Shingler, G, Mahon, D, Elgaddal, S, Payne, Cj, Shaikh, Ia, Dalmia, S, Nair, M, Finch, Jg, Chapple, K, Bawa, S, Watfah, J, Carden, Ca, Makhija, R, Rao, M, Sarveswaran, J, Vijay, V, Rekhraj, S, Knight, B, Siddiqui, Mn, Sebastian, Jf, Glen, P, Vakis, S, Ebied, H, Rajaram, R, Gray, J, Mcgrath, D, Faulkner, G, Gopalswamy, S, Varcada, M, Woodward, A, Williams, Gl, Szentpali, K, Ravindran, R, Bronder, C, Thaha, Ma, Rate, A, Shetty, Vd, Rao, V, Sajid, M, Clements, B, Patel, Rt, Mason, C, Branagan, G, Maude, K, Kaur, G, Lyons, A, Ainsworth, P, Hagger, R, Zadi, Az, Maslekar, Su, Kinross, J, Irukulla, S, Hawkins, W, Wheatstone, S, Magro, T, Bailey, S, Marshall, G, Mccullough, J, Marangoni, G, Leung, El, Borg, Cm, Gopinath, S, Kirkby-Bott, J, Yalamarthi, S, Mirza, S, Brett, M, Ramcharan, S, Pandey, V, Thava, B, Andreani, Sm, Sahay, Sj, Aravind, B, Downey, M, Nicol, D, Whitehouse, P, Sharma, A, Francis, N, Chitsabesan, P, Stewart, Dj, Norcia, Gg, Cucinotta, E, Cianchi, F, Romario, Uf, Taglietti, L, Capelli, P, Garulli, G, Parisi, A, Nitti, D, Guglielmi, A, Alonzo, A, Scandroglio, I, Moretto, G, Ansaloni, L, Pietrabissa, A, Foschi, D, Vettoretto, N, Ercolani, G, Coppola, M, Colangelo, E, Morandi, E, Niolu, P, Pala, M, Coletti, M, Pisanu, A, Nicolosi, A, Sammarco, G, Berti, S, Soliani, P, Tonini, V, Stella, M, Ceccarelli, G, De Nisco, C, Castagnoli, G, De Nardi, P, Borghi, F, Agresta, F, Benevento, A, Cantafio, S, Cesari, Mc, Rubbini, M, Chetta, G, De Marchi, F, Nora, Mf, Sousa, H, Nascimento, Ca, Casimiro, C, Costa, Sd, Rosa, Mj, Carvalho, N, Correia, J, Gomes, Ap, Hill, Ad, Walsh, Tn, Aremu, Ma, Mulsow, J, El-Masry, S, Gillick, J, Garvin, J, Caldwell, M, Mehigan, B, Peirce, Cb, Cooke, F, Mealy, K, Ruano, A, Ais, G, Fueyo, J, Parajó, Ae, Bernal-Sprekelsen, Jc, Monzón-Abad, Ja, Blanco, F, Arroyo, A, Bazán-Hinojo, Mc, Ramos-Bernado, Mi, Lopez-Ruiz, Ja, Golda, T, Julià, D, Cuadrado, Mm, Gómez-Abril, Sa, Martinez, J, Aguayo, Jl, Millan, M, Alvarez-Gallego, M, Muinelo-Lorenzo, M, Parra, Jm, Muñoz-Muñoz, E, De Chaves-Rodríguez, Pg, Cánovas-Moreno, G, Rodriguez-Lopez, M, Segura-Sampedro, Jj, García-Granero, A, Redondo-Calvo, Fj, Dyson, S, Thakur, D, Swords, C, Siaw, O, Zelazek, M, Woo, R, Badran, A, Aruparayil, N, Christopoulos, P, Chambers, B, O'Neill, N, Long, Rh, Mccaughey, P, Wong, Ml, Mccain, R, Lennox-Warburton, Hc, Moore, C, Manektella, Km, Mcilwaine, S, Rupani, S, Simpson, Dj, Wauchope, J, Ng, M, Christian, L, Crone, A, Sacks, R, Symons, N, Lazzaro, A, Patil, Sd, Roomi, S, Silva, I, Hodgson, Jm, Ly, C, Froud, H, Patel, H, Cay, P, Karwal, R, Danquah-Boateng, D, Berry, B, Esmail, Hd, Maripi, H, Bilku, D, Mckelvie, Ma, Miller, K, Maina, A, Velho, R, Hasan, R, Clingan, R, Jah, S, Waite, K, Jones, A, Buckley-Jones, S, Lecky-Thompson, L, Saghir, N, Mansoor, S, Mistry, D, Brown, R, Wong, A, Gurung, S, Wensley, F, Fleming, Ta, Griggs, R, Haines, S, Bedoya, S, Beverstock, A, Johnson, J, Govind, G, Niaz, O, Dyal, A, Tokidis, E, Punj, S, Leusink, A, Rudland, I, Kelly, M, Morgan, R, Al-Musawi, S, Lek, C, Gilbert, A, Gosal, A, Mahoney, R, Parwaiz, I, Mitchard, Mj, Ribeiro, B, Merai, H, Dean, Ea, Khan, S, Baginski, A, Mann, C, Foers, W, Jones, L, Woodward, B, Mcwhirter, Dm, Thomas, At, Gilbert, Tg, Weatherburn, Lw, Pilkington, Jp, Cameron, Fc, Clements, Jd, Mccann, C, Davidson, S, Hackney, L, Martin, A, Du, Dt, Shakoor, Z, Yen, Sk, Adnan, M, Ranathunga, S, Sana, S, Tay, Yh, Chin, My, Gillespie, M, Brown, Ag, Campbell, U, Chatzikonstantinou, M, Mahendran, B, Flack, T, Chowdhary, M, Lim, Jm, Whiteman, E, Shepherd, Ja, Pedder, A, Siggens, Kl, Lai, Cw, Morrison-Jones, V, Hayat, Z, Nehikhare, I, Macleod, C, Quinn, Hc, Brown, A, Neagle, G, Chok, Sm, Carrano, Fm, Abbassi, Oa, Divekar, Ga, Halmer, S, Adams, Re, Davies, Pl, Wong, Sy, Amarasinghe, R, Tague, Le, Jones, E, Singh, J, Boza, K, Kelly, Sd, Morrison, F, Chan, Wh, Wilson, Ej, Awokoya, Oo, Griffiths, Sn, Kirkham, En, Cotton, Ae, Adimonye, A, Leighton, Pa, Abdelrahman, A, Cartwright, H, Gates, Z, Miguras, M, Khan, K, Louw, C, Grove, T, Badenoch, T, Mckeon, J, Wood, C, Leitch, Rp, Sgardelis, P, Perera, Mi, Nagarajan, D, Malam, Y, Theodoropoulou, K, Rajagopal, S, Kaptanis, S, Popova, D, Olagbaiye, O, Tayeh, S, Rigby, S, Harris, Mp, Ren, Kz, Liaw, G, Zhou, S, White, F, Marshall, Cm, Mitchell, Jh, Anderson, Dj, Kanakala, V, Hollingsworth, A, Paramasevon, Kr, Milward, J, Ahmed, S, Fanibi, Bf, Ferguson, N, Dickson, Ea, Shaw, Av, Dixon, F, Morrish, S, Dandy, R, Fooks, P, Sharma, P, Islam, N, Tabain, V, Keegan, R, Ahel, J, Alhammali, T, Graveston, J, Balai, Ej, Rothnie, K, Pankin, Gp, Eiben, Ie, Jackson, Nj, Dhar, M, Nash, D, Dharamavaram, S, Seth, M, Chowdhury, F, Rezacova, M, Seneviratne, N, Turner, Ej, Currow, C, Isherwood, Jd, Hobson, Bm, Lui, Dh, Rodger, V, Ting, N, Photiou, D, Taze, D, Lodhia, S, Earnshaw, L, Kumar, K, Neale, A, Bastianpillai, J, Cipparrone, M, Barrie, A, Nash, Z, Anandan, L, Tailor, K, Vinnicombe, Z, Krivan, S, Kuo, R, Giorga, A, Habib, H, Malik, K, Bogdan, M, Mahon-Daly, Fp, Athersmith, Mj, Strange, Ja, Wheeler, C, Summerfield, L, Khaw, Ra, Ashour, O, Iosif, E, Fadel, M, Gopalakrishnan, K, Orme, N, Williams, S, Rashid, M, Sultana, A, Patel, N, Pearson, R, Yasin, T, Bevan, V, Al-Sarireh, B, Brown, M, Mohd, N, Howie, Ee, Poudevigne, M, Paget, C, Rallage, H, Chui, K, Fawzi, F, Layman, S, Okorocha, E, Jama, Gm, Orawiec, P, Kouli, O, Hassane, A, Kilkenny, J, Devine, Aa, Laurenson, M, Slezak, I, Barker, T, Lau, E, Limbada, M, O'Brien, J, Weaver, J, Hajibandeh, S, Shah, J, Mansour, Mm, Malik, Sn, Davis, S, Trew, F, Bandyopadhyay, Sk, Dart, K, Guru-Naidu, S, Callan, R, Nair, Mk, Alani, M, Sezen, E, Salim, S, Shurlock, J, Siddique, K, Forouzanfar, A, Brews, R, Acharya, A, Jain, A, Tozer, Pj, Warusavitarne, J, Emslie, Km, Collier-Wakefield, O, Sivaloganathan, P, Dobson, C, Elseedawy, M, Mcnally, L, Williams, M, Motiwala, Fh, Choi, S, Asmadi, Aa, Burnside, D, Everden, A, Suriyakumar, S, Sandu, L, Kent, Da, Bowen, J, Long, P, Khair, A, Shah, K, Phelan, L, Pierre, R, Dhari, Aa, Hoff, M, Nickson, S, Setshwaelo, T, Chalk, A, Parkola, Mj, Harlinska, A, Chan, T, Dudek, Jg, Rolph, R, Allen, M, Pollard, H, Gormely, R, Finlayson, H, Ljungqvist, G, Peponis, C, Rahman, M, Dhesi, S, Arshad, F, Faris, Ar, Sooriyamoorthy, T, Springate, El, Barnieh, W, Patel, A, Siddiqui, Za, Chishti, Ia, Ayube-Brown, J, Rabie, Mr, Blake, L, Yardimci, E, Nagendram, S, Neophytou, Gi, Henderson, L, Farhan-Alanie, M, Kong, Cy, Ghazala, R, Evans, J, Hussain, N, Kabir, M, Hraishawi, I, Cox, M, Bailey, Ja, Muhibullah, N, Yanni, F, Stevenson, R, Nair, A, Murphy, C, Mcgucken, O, Pandya, R, Bowerman, H, Lafaurie, G, Van Boxel, Gi, Shanmugarajah, K, Maragouthakis, D, Hanif, Z, Evans, Jd, Yoganathan, S, Richardson, Td, Cook, V, Clark, Gl, Rigney, B, O'Neill, E, Guliani, J, Chan, D, Harper, F, Sian, T, Boereboom, C, Blackwell, J, Hardy, E, Boyd-Carson, H, Couch, Dg, Barter, Ca, Thoukididou, Sn, Hatt, Jr, Jones, C, Dean, S, Rajaretnam, N, Masood, M, Thakral, N, Griffith, D, Doherty, C, Longshaw, A, Peprah, D, Mathew, G, Hook, A, Vance-Daniel, J, Ibrahim, Y, Walters, Kj, Whewell, He, Sherif, Ma, Mckenna, M, O'Sullivan, D, Woodrow, C, Gill, S, Johnstone, A, Gentry, R, Irwin, R, Forgie, A, Welsh, S, Ivey, P, Bullivant, Jk, English, Wj, Osterberg, A, Morowala, A, Al-Faham, Z, Islam, S, Tan, E, Sadek, S, Sihra, N, Shrestha, D, Chong, B, Nadeem, A, Fasuyi, Ja, Patel, Mm, Daureeawoo, R, Okekunle, B, Cheruvu, M, Mazumdar, E, Hussain, A, Patel, C, Mcquaid, M, Banks, A, Robinson, A, Khan, M, Riaz, W, Verroiotou, M, Cohen, Ja, Kouroumpas, E, Ghaffari, I, Moradzadeh, J, Kamal, M, Gulamhussein, M, Gaines, E, Ghatorae, S, Clark, S, Savill, A, Hutchinson, B, Chapman, J, Wu, F, Creasy, W, Raymond, M, Grosvenor, S, Odeh, A, Malik, Y, Bansal, H, Grant, C, Raofi, A, Ahmed, B, Mai, D, Souter, J, Hamelmann, Rn, Ikram, S, Durbacz, M, Gilliland, N, Salem, A, Chudek, D, Ladwa, N, Storey, R, Fontaine, C, Toomey, D, Miller, B, Oakey, M, Smoker, H, Chapman, Sj, O'Hagan, Sc, Tahir, W, Wilcox, G, Ahmad, A, Akram, F, Baddams, T, Boshier, Pr, Fehervari, M, Easdon, S, Ilozue, T, Adam, Me, Jokhan, S, Foster, A, Nambiar, K, Bohra, P, Janardanan, S, Shanmuganathan, V, Maqboul, F, Ettles, C, Wardle, Sd, Martinou, E, Khasria, A, Bagga, R, Motter, D, Mundkur, N, Pan, Y, Akbari, K, Farrell, Sm, Rahim, A, Gummaraju, A, Mahmoud, A, Akinsola, O, Smallcombe, N, Tarazi, M, Hanley, C, Campbell, Um, Franklin, D, Davidson, Jr, Raza, S, Krishnamoorthy, A, Rajjoub, Y, Ali, M, Seddon, Tc, Payne, Re, Das, A, Martin, Lm, Naismith, Kn, Venkata, Up, Manda, Vm, Burns, Km, Huang, J, Samuel, M, Docherty, Ja, Cheah, Wl, Ooi, R, Nyeko-Lacek, M, Marsh, L, Prideaux, A, Li, Ch, Poacher, A, Lee, M, Muzaffar, M, Kara, A, Walsh, E, Sunter, H, Roth, N, Roy, C, Mcmorran, D, Turnbull, A, Layton, Gr, Archer, Je, Yang, P, Douka, E, Amin, V, Borghol, K, Blackford, Od, Bond, S, Baker, B, Mohamed, Wo, Williams, R, Garnham, J, Robb, Hd, Allington, J, Cloney, L, Tamborska, A, Kalia, K, Fung, E, Johnston, Z, Lynch, L, Christides, A, Tan, Hl, Cynthia, G, Tsang, B, Rossi, C, Kaubrys, M, Al-Khafaji, N, Jenkins, M, Peiris, Gb, Gunning, S, Nimako, E, Pandya, D, Hever, P, Amayo, A, Bull, C, Clements, C, Al-Sheikh, M, Savioli, F, Long, M, Horsfield, E, Robertson, C, Ogboru, S, Mcilwrath, Ac, Bell, J, Limb, C, Obeid, N, Rich, Je, Balasubramaniam, A, Mashar, R, Taylor, M, Bruce, J, Dennison, G, Curtis, Nj, Ezerska, E, Ellis, B, Wiggill, S, Tee, A, Ng, S, Carder, C, Abdelwahed, A, Chandler, Sb, Tinsley, Bj, Finotti, E, Occhioni, G, Cossu, F, Vulcano, I, Viscosi, F, Michelini, M, Compagnoni, B, Sepe, C, Isolani, Sm, Regina, G, Alagna, V, Martorelli, G, Gabbianelli, C, Moroni, P, Zuin, M, Conci, S, Lazzari, G, Costamagna, D, Zurleni, Tz, Altomare, Ma, Desiderio, J, Di Cintio, A, Gemini, A, Trastulli, S, Viviani, E, Tomasoni, M, Montori, G, Harder, G, Argenti, F, Malabarba, S, Checcacci, P, Montanelli, P, Guerra, F, Skalamera, I, Staderini, F, Grandi, S, Nelli, T, Coratti, F, Sorrentino, L, Maffioli, A, Cavallo, D, Bondurri, A, Groppo, G, Curti, R, Solaini, L, Xidas, A, Manias, T, Delogu, D, Vacca, A, Solinas, L, Corbellini, C, Fiore, L, Nigro, A, Santurro, L, Angrisani, M, Sparta, C, Lorettu, A, Mura, Fa, Ruggiu, Gv, Pirari, Pf, Pau, R, Melis, M, Piu, F, Patti, S, Deserra, A, Angelieri, D, Del Basso, C, Rossi, D, Iannone, I, De Padua, C, Giubilo, C, Falaschi, F, Cirillo, B, Gordini, L, Podda, F, Sanna, S, Saba, A, Poillucci, G, Pinna, E, Messina, A, Sena, G, Cardona, R, De Luca, E, Sacco, R, Vescio, G, Ammendola, M, Romano, R, Bianco, A, Bonfante, P, D'Ambra, L, Feleppa, C, Gennai, A, Lizzi, V, Moggia, E, Imperatore, M, Bolzon, S, Belvedere, A, Amaducci, E, Ripoli, Mc, Segalini, E, Cervellera, M, Vaccari, S, Eretta, Co, O'Neill, R, Llewelyn, O, Jones, N, Clerici, F, Ballabio, M, Andolfi, E, Angelini, M, Fontani, A, Miranda, E, Scricciolo, M, Provenza, G, Pellicanò, Ga, Pulighe, F, Argenio, G, Melis, A, Balestra, F, Anania, M, Cruccu, A, Massaiu, C, Murru, Ml, Martino, A, Luzzi, Ap, La Valle, G, Chillitupa, Cz, Bartoli, A, Conti, D, Spaziani, A, Bellochi, R, Listorti, C, Salandini, Mc, Carlucci, M, Tenconi, Sm, Cannavò, M, Marano, A, Giuffrida, Mc, Cannata, G, Pellegrino, L, Giraudo, G, Baraghini, M, Garzi, A, Giudicissi, R, Zalla, T, Romoli, L, Vannucchi, A, Giani, I, Feroci, F, Calussi, M, Ribaudo, M, Fiorot, A, Stecca, T, Nistri, C, Fornasier, C, Valiani, Sv, Brunelli, Db, Evoli, Le, Giuliani, Ng, Contine, Ac, Renzi, Cr, Feo, Cv, Anania, G, Carcoforo, P, Aisoni, F, Licari, L, Tutino, R, Cocorullo, G, Silvestri, V, De Marco, P, Fontana, T, Orlando, G, Falco, N, Baseggio, M, Napetti, S, Mella, A, Rossi, Gm, Chimetto, A, Cosci, M, Bonomo, M, Scialandrone, G, Chetta, N, Carvalho, Lc, Magalhães, J, Pereira, Am, Fernandes, C, Fareleira, A, Gonçalves, D, Pais, M, Pereira, A, Resende, Fm, Correia, D, Cardoso, D, Tojal, A, Santos, Sc, Barbosa, L, Louro, Hc, Bairos, F, Martins, Fm, Messias, Fm, Ferreira, M, Borges, Fc, Botelho, P, Lima, M, Valente, Pm, João, Aa, Guimarães, Jm, Rocha, R, Nogueira, St, Kabir, U, Wong, C, Rahmani, L, Tan, S, Chng, S, Jasinski, B, Cheng, Sa, Mardhiah, S, Mcglynn, K, Hannan, E, Burke, J, Haveliwala, Z, O'Neill, M, Boland, M, Hayes, C, Fox, A, Zaborowski, A, Mitru, Rm, Mc-Dermott, A, Coyle, D, Stoica, I, Mcmahon, Sv, Laughlin, Dm, Kannegieser-Bailey, M, Murphy, R, Muntean, A, Shet, S, Thomas, L, De Freitas, S, Quill, S, Aljorfi, A, Soh, B, Law, Jj, Hartnett, J, Jansen, T, Gilgan, J, Jung, J, Scanlon, K, Szucs, A, Ahern, Dp, Redmond, Ae, Edwards, Se, Manoharan, P, Brennan, S, Abdelgadir, Am, Mckevitt, Kl, Zarog, Ma, Ahmed, G, Bukhari, W, Ahad, A, Paniagua, M, Samartin, C, Primo, Jc, Garrido, L, Lopez, M, Rufo, E, Trostchansky, I, Rodriguez, L, Infante, H, Acosta, A, Cremades, P, Cidoncha, A, Olmos, V, Oliva, I, Santamaria, C, Cavero, A, Calvo, H, Suero, Ca, Maderuelo, Vm, Galvez, P, Hernando, A, Eguaras, I, Recreo, Ac, García-Carrero, M, Moreda, R, De Andres, U, Del Pozo, E, Calvo, M, Moratalla, Cn, Ronda, Rn, Contreras, Rg, De Burgos, Cb, Cortés, Gv, Martínez, Cc, Agudo, Ar, Soriano, Jt, Ramos, Xh, Echazarreta, E, Elia, M, Hernaez, A, Sanchez, L, Vallejo-Bernad, C, Oliver, Jr, Sánchez-Rubio, M, Kälviäinen, Hk, Genzor, S, González-Nicolás, T, Puerta, E, Laviano, E, Gimenez, T, Fermiñán, A, Muriel-Álvarez, P, Sierra-Grañón, Je, Escoll-Rufino, J, Cuello-Guzmán, E, Mestres-Petit, N, Merichal-Resina, M, Pinillos-Somalo, A, Gomez-Carmona, Z, Vazquez-Fernandez, Ap, Trujillo-Diaz, Jj, Couso, Jr, Fernández, Md, Riera, E, Espinosa, J, Carral-Freire, M, Martínez-Almeida, R, Santarrufina-Martínez, S, Sebastián-Tomás, Jc, Gonzálvez-Guardiola, P, Fernández, Ec, Mozo, A, Stoyanov, Ti, Santamaría, Pc, Grimaldo, Eg, Fernández-Candela, A, Curtis-Martínez, C, Del-Valle-Ruiz, Sr, Sánchez-Cifuentes, A, Ramírez-Faraco, M, López, Af, Leon, C, Kumar, S, Fornell-Ariza, M, Ayllón-Gámez, S, Peña-Barturen, C, Ojea-Ruiz-Yherla, L, Saavedra-Chacón, M, Perez-Calvo, J, Gomez-Facundo, H, Riba-Combatti, L, Manas, Oc, De-Soto-Cardenal, B, De-La-Herranz-Guerrero, P, Dominguez-Sanchez, C, Gamero-Huaman, Jc, Suarez-Cabrera, A, Ramirez-Redondo, Aa, Lara-Fernandez, Y, Bascuas-Rodrigo, B, Lopez-Duran, Bl, Pigem, A, Gil, J, Salvador, H, Planellas, P, Farrés, R, Caballero, A, Arnau, M, Tapiolas, I, Ridaura, N, Roncero, L, Collado-Roura, F, Fijo, Lm, Cormenzana, Ob, Viñas, Nl, Grifell, M, Prats, Ma, Torrado, Aa, Sanz-Navarro, S, Contreras-Saiz, E, Solar-García, L, Moreno-Gijón, M, Suárez-Sánchez, A, Díaz-Vico, T, Rodicio-Miravalles, Jl, García-Gutierrez, C, Pila, U, Melone, S, Martin-Prieto, L, Rojo, Ja, Gonzalez, M, Zorrilla, L, Garcia-Marin, Ja, Baeza-Murcia, M, Pellicer-Franco, E, Jimenez-Ballester, Ma, Asensio-Gomez, L, Gortazar-De-Las-Casas, S, Guevara-Martinez, J, Ramirez, L, Verea, S, Anguita, F, Navarro, G, Criado, Adc, Lara, Mc, Martinez, Et, Sanchez-Martinez, A, Hernandez-Gimenez, L, Galofre-Recasens, M, Ferrer-Vilela, I, Pérez-Sanchez, Le, Esteves, Mb, Menéndez-Moreno, A, Baz-Figueroa, C, Rosat, A, Hontoria, M, García, Na, Gracia-Roman, R, Pascua-Sole, M, Pino-Perez, O, García-Pérez, Jm, Pineño-Flores, C, Ambrona-Zafra, D, Sancho-Muriel, J, Alvarez, E, Jiménez-Rosellón, R, Daga, O, Alberca-Paramo, A, Sanchez-Garcia, S, García-Santos, E, Pareja-Ciuró, F, Olivares-Oliver, C, Navarro-Morales, L, Tamayo-López, Mj, Tinoco-González, J, García-Rivera, Co, Agua, Ia, Moreno-Suero, F, Pereira-Mosquera, E, Zerpa, C, Llacer, E, Diaz, A, Caro, A, Feliu, F, Franco, M, Escuder, J, Abellan, M, Padilla, E, Mambrilla-Herrero, S, Plua-Muniz, Kt, Bailon-Cuadrado, M, Tejero-Pintor, Fj, Choolani-Bhojwani, E, Vila-Zarate, C, Delgado-Plasencia, Lj, Ponchietti, L, Cousins, L, Busuttil, A, Baird, C, Drye, N, Brown, Od, Mansour, S, Anderson, O, Mahapatra, R, Clements, Ja, D'Souza, N, Littlehales, Dj, Tang, Am, Byrne, Be, Cunha, P, Ogbuokiri, C, Eiben, P, Gravante, G, Kho, H, Dobbs, S, Doulias, T, Ng, J, Wilson, M, Venugopal, R, Wolff, J, Akhtar, K, Walji, Hd, Tognarelli, Jm, Knight, Ka, Ansari, A, Hussaini, Sa, Wright, E, Brewer, H, Rinkoff, S, Harries, Rl, Fairfield, Cj, Abbott, T, Jackson, A, Wright, Hl, Walters, U, Carney, K, Logan, Pc, Mughal, Z, Strachan, E, Chasty, B, Ma, J, Mazzeo, C, Badii, B, Armellini, A, Grassia, M, Perin, A, Ruzzenente, A, Magnoli, M, Depalma, N, Longheu, A, Papandrea, M, Dova, L, De Prizio, M, Gusai, Gp, Di Zitti, L, Geretto, P, Azabdaftari, A, Chianese, G, Elbetti, C, Ruffolo, C, Giaccari, S, Devezas, V, Ferreira, J, Peixoto, R, Alshafei, A, Simo, V, José, H, Ugarte-Sierra, B, Salva, Ab, Gómez, N, Marinello, F, Medina-Arana, V, Vega, L, Ballester, Mm, Espina, B, Prieto-Nieto, Mi, Rodríguez, Ec, Padilla-Valverde, D, Duran-Muñoz-Cruzado, Vm., Bhangu A., Nepogodiev D., Matthews J.H., Morley G.L., Naumann D.N., Ball A., Chauhan P., Bhanderi S., Mohamed I., Glasbey J.C., Wilkin R., Drake T.M., Clements J., Blencowe N.S., Herrod P., Pata F., Frasson M., Blanco-Colino R., Soares A.S., Jain S., Amuthalingam T., Tyler R., Griffiths E.A., Pinkney T.D., Gee O., Morton D.G., Beggs A., Beral D., Bowley D., Cruickshank N., Daniels I., Griffiths E., Hornby S.T., Lund J.N., Marriott P., Singh P., Smart N.J., Speake D., Thompson C., Torkington J., Torrance A., Vohra R., Warren O., Winter D.C., Pellino G., Sgro A., Simioni A., Farina V., Podda M., Di Saverio S., Birindelli A., Pasquali S., Surg I.T., Surg P.T., Bolton W., Bradshaw C.J., Chean C.S., Harris G., Haddow J.B., Jamieson N.B., McCain S., Mason J., Milgrom D., Nana G.R., Mohamed M.N., Brien J.O., Pearce J., Rabie M., Sahnan K., Sarmah P., Skerritt C., Ghazanfar M.A., Sreedharan L., Kabwama S., Gray R.T., Kamande I.W., Nazarian S., Dar F.A., Misky A.T., Arunachalam S., Twum-Barima C.S., Mohamed I.M., Connor K.L., Coe P.O., Kosti A., Elshaer M., Colvin D.A., Charalambous M.P., Yeung K., Merker L., Morrison T., Thaventhiran A.J., Gilbert T.M., Clements J.M., Hicks G., Afshar S., Mckinley N.C., Assaf N., Hanna T., Macinnes E., Thavanesan N., Dubois A.S., Palani-Velu L.K., Tezas S., Yow L., Radwan R.W., Abdelrahman M., Lee K.A., Zarka Z.A., Mcdowall N.A., Tan C.Y., Venn M.L., Ashmore D.L., Whitehorn S.E., Golder A.M., Reddy A., Delimpalta C., Kay O.H., Shah S.M., Eiben I., Doyle C., Tudyka V., Issa E., West H., Brewer H.K., Farrow E.Z., Taylor N.S., Smart C.J., Griffiths N.P., Halkias C., Vitish-Sharma P., Knight S.R., Mowbray N.G., Olivier J.B., Lee K.J., Clement K.D., Chrastek D., Panda N., Connor M.J., Fahmy S.E., Bryan E.S., Ngu W.S., Adegbola S.O., Vaughan E.M., Stupalkowska W., Simmonds L., Malik A., Hussein A., Karim M.J., Singhal T., Ormiston R., Kung V., Rabie M.A., Park J.H., Lal N., Worku D., D'Auria M., Ang A., Orizu M., Gammeri E., Clough E., Choy C.H., Lawday S., Hann A.J., Robinson D., Wardle B.G., Mcdonnell D., Rutherford D.G., Hickey L.M., Garg A.G., Rezvani S., Bell C.R., Mahmood F., Rehman S., Donaldson G., Peleki A., Pearce L., Sharp O.L., Singh S., Thompson D.B., El-Tayar O., Hollyman M., Rupasinghe S.N., Toomey D.B., Murray M.P., Amtul N., Mersh R.J., Newton R.C., Al-Khyatt W., Stephens G.F., Abbas S.H., Iqbal M.R., Brown C.E., Renshaw S., Hureibi K.A., Pullabatla-Venkata U.P., Donohoe N.O., Myatt A., Egan R.J., Rangarajan K., Trail M., Mckay S.C., Engall N., Jerome E., Townsend D.C., Patel B.Y., Pronin S., Chandratreya N., Choong J.H., Mohamed T.M., Hudson-Peacock N.J., Manson R., Hebbar K., Mothe B.S., Weegenaar C.R., Saad M., Bowman C.R., Serventi F., Fleres F., Foppa C., Pata G., Baronio G., Pertile D., Lucchi A., Sagnotta A., Maretto I., Campagnaro T., Gatti M., Gjoni E., Roscio F., Inama M., Coccolini F., Colombo F., Avanzolini A., Aresu S., De-Manzoni-Garberini A., Merlini D.A., Chessa A., Tamini N., Mulas S., Cillara N., Coletta D., Atzeni J., Erdas E., Gallo G., Francone E., Di Gioia P., Bianchi C.L., Ferrara F., Biancafarina A., Scabini S., Marano L., Miegge A., Sasia D., Savino G., Scatizzi M., D'Amico F.E., Arcuri G.A., Gavagna L., Salamone G., Tatulli F., Goldin E., Matos M.L., Caldeira A.B., Romano J., Pereira J., Azevedo J., Azevedo J.M., Simoes J., Silva A., O'Leary D.P., Kennedy N.D., Quinn E.M., Zhang A.Y., Neary P.M., De-Marchi J.A., O'Connor B.R., Wijesundera K., Foley N.M., Wong J., Tiedt L.A., Bolger J.C., Connelly T.M., Ahmed O.S., Vigorita V., Garcia V., Arredondo J., Redondo E., Sainz B., Aldrey I., Landaluce-Olavarria A., Gomez A.A., Cordoba E., Sanchez-Fuentes M.N., Cerdan-Santacruz C., Beltran-De-Heredia J., Garcia M., Veres T., Garcia-Novoa A., Abellan A.M., Garcia-Catala L., Ruiz-Marin M., Menendez P., Roldan-Ortiz S., Navas-Cuellar J.A., Sabia D., Gomez-Rosado J.C., Navidad M.S., Caula C., Sanchez E.R., Espin-Basany E., Fernandez-Martinez D., Bravo-Gutierrez A.F., Paya-Llorente C., Dujovne P., Lima F., Soria-Aledo V., Gomez C.J., Pascual-Miguelanez I., Muinelo M., Alvarez C.M., Vargas-Pierola H.J., Vallve-Bernal M., Hidalgo-Rosas J.M., Arenal-Vera J.J., Sena-Ruiz F., Sanchez-Guillen L., Villarejo-Campos P., Tallon-Aguilar L., Garcea A., Bennett J.M., Whittaker L., Gidwani A.L., Byrnes C.K., Saunders S., Shiwani M.H., Ashraf N., Venkatasubramaniam A.K., Bevan K.E., Mcarthur D., Mustafa A.K., Griffith J.P., Blazeby J.M., Charalabopoulos A., Campbell W., Reese G., Warren O.J., Peacock M., Menzies D., Jenner D., Eardley N.J., Yoong S., Abulafi M., Avalapati H., Thompson R., Nastro P., Kochupapy R., Stubbs B.M., McIntyre R., Crozier J., Patel P.K., Pento V., Beasley W.D., Roxburgh C., Youssef H., Alexander R., Denley S., Di Franco F., Quddus A., Saha A., Hunter I., Hannay J., Velchuru V.R., Bond-Smith G., Salama Y., Bhargava A., Panagiotopoulos S.P., Watson N., Garcea G., Boddy A.P., Dunning P.G., Lloyd G., Gurjar S.V., Hill J., Andrews B., Singh A., Ruzvidzo F., Shingler G., Mahon D., Elgaddal S., Payne C.J., Shaikh I.A., Dalmia S., Nair M.S., Finch J.G., Chapple K.S., Bawa S., Watfah J., Carden C.A., Makhija R., Rao M., Sarveswaran J., Vijay V., Rekhraj S., Knight B., Siddiqui M.N., Sebastian J.F., Glen P., Vakis S., Ebied H., Rajaram R., Gray J., Mcgrath D., Faulkner G., Gopalswamy S., Varcada M., Woodward A., Williams G.L., Szentpali K., Ravindran R., Bronder C., Thaha M.A., Rate A., Shetty V.D., Rao V., Sajid M.S., Clements B., Patel R.T., Mason C., Branagan G., Maude K., Kaur G., Lyons A., Ainsworth P., Hagger R., Zadi A.Z., Maslekar S.U., Kinross J., Irukulla S., Hawkins W., Wheatstone S., Magro T., Bailey S., Marshall G., Mccullough J., Marangoni G., Leung E.L., Borg C.M., Gopinath S., Kirkby-Bott J., Yalamarthi S., Mirza S., Brett M., Ramcharan S., Pandey V., Thava B., Andreani S.M., Sahay S.J., Aravind B., Downey M., Nicol D., Whitehouse P., Sharma A., Francis N., Chitsabesan P., Stewart D.J., Norcia G.G., Cucinotta E., Cianchi F., Romario U.F., Taglietti L., Capelli P., Garulli G., Parisi A., Nitti D., Guglielmi A., Alonzo A., Scandroglio I.S., Moretto G., Ansaloni L., Pietrabissa A., Foschi D., Vettoretto N., Ercolani G., Coppola M., Colangelo E., Morandi E., Niolu P., Pala M., Coletti M., Pisanu A., Nicolosi A., Sammarco G., Berti S., Soliani P., Tonini V., Stella M., Ceccarelli G., De Nisco C., Castagnoli G., De Nardi P., Borghi F., Agresta F., Benevento A., Cantafio S., Cesari M.C., Rubbini M., Chetta G., De Marchi F., Nora M.F., Sousa H.S., Nascimento C.A., Casimiro C., Costa S.D., Rosa M.J., Carvalho N., Correia J., Gomes A.P., Hill A.D., Walsh T.N., Aremu M.A., Mulsow J., El-Masry S., Gillick J., Garvin J., Caldwell M., Mehigan B., Peirce C.B., Cooke F., Mealy K., Ruano A., Ais G., Fueyo J., Parajo A.E., Bernal-Sprekelsen J.C., Monzon-Abad J.A., Blanco F., Arroyo A., Bazan-Hinojo M.C., Ramos-Bernado M.I., Lopez-Ruiz J.A., Golda T., Julia D., Cuadrado M.M., Gomez-Abril S.A., Martinez J., Aguayo J.L., Millan M., Alvarez-Gallego M., Muinelo-Lorenzo M., Parra J.M., Munoz-Munoz E., De Chaves-Rodriguez P.G., Canovas-Moreno G., Rodriguez-Lopez M., Segura-Sampedro J.J., Garcia-Granero A., Redondo-Calvo F.J., Dyson S., Thakur D., Swords C., Siaw O., Zelazek M., Woo R., Badran A., Aruparayil N., Christopoulos P., Chambers B., O'Neill N., Long R.H., Mccaughey P., Wong M.L., Mccain R.S., Lennox-Warburton H.C., Moore C., Manektella K.M., Mcilwaine S., Rupani S., Simpson D.J., Wauchope J., Ng M., Christian L., Crone A., Sacks R., Symons N., Lazzaro A., Patil S.D., Roomi S., Silva I., Hodgson J.M., Ly C., Froud H., Patel H., Cay P., Karwal R.S., Danquah-Boateng D., Berry B., Esmail H.D., Maripi H., Bilku D., McKelvie M.A., Miller K., Maina A., Velho R., Hasan R., Clingan R., Jah S., Waite K., Jones A., Buckley-Jones S., Lecky-Thompson L., Saghir N., Mansoor S., Mistry D., Brown R., Wong A., Gurung S., Wensley F., Fleming T.A., Griggs R., Haines S., Bedoya S., Beverstock A., Johnson J., Govind G., Niaz O., Dyal A., Tokidis E., Punj S., Leusink A., Rudland I., Kelly M., Morgan R., Al-Musawi S., Lek C., Gilbert A., Gosal A., Mahoney R., Parwaiz I., Mitchard M.J., Ribeiro B., Merai H., Dean E.A., Khan S., Baginski A., Mann C., Foers W., Jones L., Woodward B., Mcwhirter D.M., Thomas A.T., Gilbert T.G., Weatherburn L.W., Pilkington J.P., Cameron F.C., Clements J.D., Mccann C., Davidson S., Hackney L., Clements J.S., Martin A., Du D.T., Shakoor Z., Yen S.K., Adnan M., Ranathunga S., Sana S., Tay Y.H., Chin M.Y., Gillespie M., Brown A.G., Campbell U., Chatzikonstantinou M., Mahendran B., Flack T., Chowdhary M., Lim J.M., Whiteman E., Shepherd J.A., Pedder A., Siggens K.L., Lai C.W., Morrison-Jones V., Hayat Z., Nehikhare I., Macleod C., Quinn H.C., Brown A., Neagle G., Chok S.M., Carrano F.M., Abbassi O.A., Divekar G.A., Halmer S., Adams R.E., Davies P.L., Wong S.Y., Amarasinghe R., Tague L.E., Jones E., Singh J., Boza K., Kelly S.D., Morrison F., Chan W.H., Wilson E.J., Awokoya O.O., Griffiths S.N., Kirkham E.N., Cotton A.E., Adimonye A., Leighton P.A., Abdelrahman A., Cartwright H., Gates Z., Miguras M., Khan K., Louw C., Grove T., Badenoch T., Mckeon J., Wood C.S., Leitch R.P., Sgardelis P., Perera M.I., Nagarajan D., Malam Y., Theodoropoulou K., Rajagopal S., Kaptanis S., Popova D., Olagbaiye O., Tayeh S., Rigby S., Harris M.P., Ren K.Z., Liaw G., Zhou S., White F., Marshall C.M., Mitchell J.H., Anderson D.J., Kanakala V., Hollingsworth A., Paramasevon K.R., Milward J., Ahmed S., Fanibi B.F., Ferguson N., Dickson E.A., Shaw A.V., Dixon F., Morrish S., Dandy R., Fooks P., Sharma P., Islam N., Tabain V., Keegan R., Ahel J., Alhammali T., Graveston J., Balai E.J., Rothnie K., Pankin G.P., Eiben I.E., Jackson N.J., Dhar M., Nash D., Dharamavaram S., Seth M., Chowdhury F., Rezacova M., Seneviratne N., Turner E.J., Currow C., Isherwood J.D., Hobson B.M., Lui D.H., Rodger V., Ting N., Photiou D., Taze D., Lodhia S., Earnshaw L., Kumar K., Neale A., Bastianpillai J., Cipparrone M., Barrie A., Nash Z., Anandan L., Tailor K., Vinnicombe Z., Krivan S., Kuo R., Giorga A., Habib H., Malik K., Bogdan M., Mahon-Daly F.P., Athersmith M.J., Strange J.A., Wheeler C., Summerfield L., Khaw R.A., Ashour O., Iosif E., Fadel M., Gopalakrishnan K., Orme N., Williams S., Rashid M., Sultana A., Patel N., Pearson R., Yasin T., Bevan V., Al-Sarireh B., Brown M., Mohd N., Howie E.E., Poudevigne M., Paget C., Rallage H., Chui K., Fawzi F., Layman S., Okorocha E., Jama G.M., Orawiec P., Kouli O., Hassane A., Kilkenny J., Devine A.A., Laurenson M., Slezak I., Barker T., Lau E., Limbada M., O'Brien J., Weaver J., Hajibandeh S., Shah J., Mansour M.M., Malik S.N., Davis S., Trew F., Bandyopadhyay S.K., Dart K., Guru-Naidu S., Callan R., Nair M.K., Alani M., Sezen E., Salim S., Shurlock J., Siddique K., Forouzanfar A., Brews R., Acharya A., Jain A., Tozer P.J., Warusavitarne J., Emslie K.M., Collier-Wakefield O., Sivaloganathan P., Dobson C., Elseedawy M., McNally L., Williams M., Motiwala F.H., Choi S., Asmadi A.A., Burnside D., Everden A., Suriyakumar S., Sandu L., Kent D.A., Bowen J., Long P., Khair A., Shah K., Phelan L., Pierre R., Dhari A.A., Hoff M., Nickson S., Setshwaelo T., Chalk A., Parkola M.J., Harlinska A., Chan T., Dudek J.G., Rolph R., Allen M., Pollard H., Gormely R., Finlayson H., Ljungqvist G., Peponis C., Rahman M., Dhesi S., Arshad F., Faris A.R., Sooriyamoorthy T., Springate E.L., Barnieh W., Patel A.S., Siddiqui Z.A., Chishti I.A., Ayube-Brown J., Rabie M.R., Blake L., Yardimci E., Nagendram S., Neophytou G.I., Henderson L., Farhan-Alanie M., Kong C.Y., Ghazala R., Evans J., Hussain N., Kabir M., Hraishawi I., Cox M., Bailey J.A., Muhibullah N., Yanni F., Stevenson R., Nair A., Murphy C., Mcgucken O., Pandya R., Bowerman H., Lafaurie G., Van Boxel G.I., Shanmugarajah K., Maragouthakis D., Hanif Z., Evans J.D., Yoganathan S., Richardson T.D., Cook V., Clark G.L., Rigney B., O'Neill E., Guliani J., Chan D., Harper F., Sian T., Boereboom C., Blackwell J., Hardy E., Boyd-Carson H., Couch D.G., Barter C.A., Thoukididou S.N., Hatt J.R., Jones C.S., Dean S., Rajaretnam N., Masood M., Thakral N., Griffith D., Doherty C., Longshaw A., Peprah D., Mathew G., Hook A., Vance-Daniel J., Ibrahim Y., Walters K.J., Whewell H.E., Sherif M.A., Mckenna M., O'Sullivan D., Woodrow C., Gill S., Johnstone A., Gentry R., Irwin R., Forgie A., Welsh S., Ivey P., Bullivant J.K., English W.J., Osterberg A., Morowala A., Al-Faham Z., Islam S., Tan E., Sadek S., Sihra N., Shrestha D., Chong B., Nadeem A., Fasuyi J.A., Patel M.M., Daureeawoo R., Okekunle B., Cheruvu M., Mazumdar E., Hussain A., Patel C., Mcquaid M., Banks A., Robinson A., Khan M.S., Riaz W., Verroiotou M., Cohen J.A., Kouroumpas E., Ghaffari I., Moradzadeh J., Kamal M., Gulamhussein M., Gaines E., Ghatorae S., Clark S., Savill A., Hutchinson B., Chapman J., Wu F., Creasy W., Raymond M., Grosvenor S., Odeh A., Malik Y., Bansal H., Grant C., Raofi A., Ahmed B., Mai D., Souter J., Hamelmann R.N., Ikram S., Durbacz M., Gilliland N., Salem A., Chudek D., Ladwa N., Storey R., Fontaine C., Toomey D., Miller B., Oakey M., Smoker H., Chapman S.J., O'Hagan S.C., Tahir W., Wilcox G., Ahmad A., Akram F., Baddams T.S., Boshier P.R., Fehervari M., Easdon S., Ilozue T., Adam M.E., Jokhan S., Foster A., Nambiar K., Bohra P., Janardanan S., Shanmuganathan V., Maqboul F., Ettles C., Wardle S.D., Martinou E., Khasria A., Bagga R., Motter D., Mundkur N., Pan Y., Akbari K., Farrell S.M., Rahim A., Gummaraju A., Mahmoud A., Akinsola O., Smallcombe N., Tarazi M., Hanley C., Campbell U.M., Franklin D., Davidson J.R., Raza S.S., Krishnamoorthy A., Rajjoub Y., Ali M., Seddon T.C., Payne R.E., Das A., Martin L.M., Naismith K.N., Venkata U.P., Manda V.M., Burns K.M., Huang J., Samuel M., Docherty J.A., Cheah W.L., Ooi R., Nyeko-Lacek M., Marsh L., Prideaux A., Li C.H., Poacher A., Lee M., Muzaffar M., Kara A., Walsh E., Sunter H., Roth N., Roy C., Mcmorran D., Turnbull A., Layton G.R., Archer J.E., Yang P., Douka E., Amin V., Borghol K., Blackford O.D., Bond S., Baker B., Mohamed W.O., Williams R., Garnham J., Robb H.D., Allington J., Cloney L., Tamborska A., Kalia K., Fung E., Johnston Z., Lynch L., Christides A., Tan H.L., Cynthia G., Tsang B., Rossi C., Kaubrys M., Al-Khafaji N., Jenkins M., Peiris G.B., Gunning S., Nimako E., Pandya D., Hever P., Amayo A., Bull C., Clements C., Al-Sheikh M., Savioli F., Long M., Horsfield E., Robertson C., Ogboru S., Mcilwrath A.C., Bell J., Limb C., Obeid N., Rich J.E., Balasubramaniam A., Mashar R., Taylor M., Bruce J.S., Dennison G., Curtis N.J., Ezerska E., Ellis B., Wiggill S., Tee A., Ng S., Carder C., Abdelwahed A., Chandler S.B., Tinsley B.J., Finotti E., Occhioni G., Cossu F., Vulcano I., Viscosi F., Michelini M., Compagnoni B., Sepe C., Isolani S.M., Regina G., Alagna V., Martorelli G., Gabbianelli C., Moroni P., Zuin M., Conci S., Lazzari G., Costamagna D., Zurleni T.Z., Altomare M.A., Desiderio J., Di Cintio A., Gemini A., Trastulli S., Viviani E., Tomasoni M., Montori G., Harder G., Argenti F., Malabarba S., Checcacci P., Montanelli P., Guerra F., Skalamera I., Staderini F., Grandi S., Nelli T., Coratti F., Sorrentino L., Maffioli A., Cavallo D., Bondurri A., Groppo G., Curti R., Solaini L., Xidas A., Manias T., Delogu D., Vacca A., Solinas L., Corbellini C., Fiore L., Nigro A., Santurro L., Angrisani M., Sparta C., Lorettu A., Mura F.A., Ruggiu G.V., Pirari P.F., Pau R., Melis M., Piu F., Patti S., Deserra A., Angelieri D., Del Basso C., Rossi D., Iannone I., De Padua C., Giubilo C., Falaschi F., Cirillo B., Gordini L., Podda F., Sanna S., Saba A., Poillucci G., Pinna E., Messina A., Sena G., Cardona R., De Luca E., Sacco R., Vescio G., Ammendola M., Romano R., Bianco A., Bonfante P., D'Ambra L., Feleppa C., Gennai A., Lizzi V., Moggia E., Imperatore M., Bolzon S., Belvedere A., Amaducci E., Ripoli M.C., Segalini E., Cervellera M., Vaccari S., Eretta C.O., O'Neill R., Llewelyn O., Jones N., Clerici F., Ballabio M., Andolfi E., Angelini M., Fontani A., Miranda E., Scricciolo M., Provenza G., Pellicano G.A., Pulighe F., Argenio G., Melis A., Balestra F., Anania M., Cruccu A., Massaiu C., Murru M.L., Martino A., Luzzi A.P., La Valle G., Chillitupa C.Z., Bartoli A., Conti D., Spaziani A., Bellochi R., Listorti C., Salandini M.C., Carlucci M., Tenconi S.M., Cannavo M., Marano A., Giuffrida M.C., Cannata G., Pellegrino L., Giraudo G., Baraghini M., Garzi A., Giudicissi R., Zalla T., Romoli L., Vannucchi A., Giani I., Feroci F., Calussi M., Ribaudo M., Fiorot A., Stecca T., Nistri C., Fornasier C., Valiani S.V., Brunelli D.B., Evoli L.E., Giuliani N.G., Contine A.C., Renzi C.R., Feo C.V., Anania G., Carcoforo P., Aisoni F., Licari L., Tutino R., Cocorullo G., Silvestri V., De Marco P., Fontana T., Orlando G., Falco N., Baseggio M., Napetti S., Mella A., Rossi G.M., Chimetto A., Cosci M., Bonomo M., Scialandrone G., Chetta N., Carvalho L.C., Magalhaes J.S., Pereira A.M., Fernandes C., Fareleira A., Goncalves D., Pais M., Pereira A., Resende F.M., Correia D., Cardoso D., Tojal A., Santos S.C., Barbosa L., Louro H.C., Bairos F., Martins F.M., Messias F.M., Ferreira M.S., Borges F.C., Botelho P., Lima M., Valente P.M., Joao A.A., Guimaraes J.M., Rocha R., Nogueira S.T., Kabir U., Wong C., Rahmani L.S., Tan S., Chng S., Jasinski B., Cheng S.A., Mardhiah S., McGlynn K., Hannan E., Burke J., Haveliwala Z., O'Neill M., Boland M., Hayes C., Fox A., Zaborowski A., Mitru R.M., Mc-Dermott A., Coyle D., Stoica I., McMahon S.V., Laughlin D.M., Kannegieser-Bailey M., Murphy R., Muntean A., Shet S., Thomas L., De Freitas S., Quill S., Aljorfi A., Soh B., Law J.J., Hartnett J., Jansen T., Gilgan J., Jung J., Scanlon K., Szucs A., Ahern D.P., Redmond A.E., Edwards S.E., Manoharan P., Brennan S., Abdelgadir A.M., Mckevitt K.L., Zarog M.A., Ahmed G., Bukhari W., Ahad A., Paniagua M., Samartin C., Primo J.C., Garrido L., Lopez M., Rufo E., Trostchansky I., Rodriguez L., Infante H., Acosta A., Cremades P., Cidoncha A., Olmos V., Oliva I., Santamaria C., Cavero A., Calvo H., Suero C.A., Maderuelo V.M., Galvez P., Hernando A., Eguaras I., Recreo A.C., Garcia-Carrero M., Moreda R., De Andres U., Del Pozo E., Calvo M., Moratalla C.N., Ronda R.N., Contreras R.G., De Burgos C.B., Cortes G.V., Martinez C.C., Agudo A.R., Soriano J.T., Ramos X.H., Echazarreta E., Elia M., Hernaez A., Sanchez L., Vallejo-Bernad C., Oliver J.R., Sanchez-Rubio M., Kalviainen H.K., Genzor S., Gonzalez-Nicolas T., Puerta E., Laviano E., Gimenez T., Ferminan A., Muriel-Alvarez P., Sierra-Granon J.E., Escoll-Rufino J., Cuello-Guzman E., Mestres-Petit N., Merichal-Resina M., Pinillos-Somalo A., Gomez-Carmona Z., Vazquez-Fernandez A.P., Trujillo-Diaz J.J., Couso J.R., Fernandez M.D., Riera E., Espinosa J., Carral-Freire M., Martinez-Almeida R., Santarrufina-Martinez S., Sebastian-Tomas J.C., Gonzalvez-Guardiola P., Fernandez E.C., Mozo A.S., Stoyanov T.I., Santamaria P.C., Grimaldo E.G., Fernandez-Candela A., Curtis-Martinez C., Del-Valle-Ruiz S.R., Sanchez-Cifuentes A., Ramirez-Faraco M., Lopez A.F., Leon C., Kumar S., Fornell-Ariza M., Ayllon-Gamez S., Pena-Barturen C., Ojea-Ruiz-Yherla L., Saavedra-Chacon M., Perez-Calvo J., Gomez-Facundo H., Riba-Combatti L., Manas O.C., De-Soto-Cardenal B., De-La-Herranz-Guerrero P., Dominguez-Sanchez C., Gamero-Huaman J.C., Suarez-Cabrera A., Ramirez-Redondo A.A., Lara-Fernandez Y., Bascuas-Rodrigo B., Lopez-Duran B.L., Pigem A., Gil J., Salvador H., Planellas P., Farres R., Caballero A., Arnau M., Tapiolas I., Ridaura N., Roncero L.S., Collado-Roura F., Fijo L.M., Cormenzana O.B., Vinas N.L., Grifell M.S., Prats M.A., Torrado A.A., Sanz-Navarro S., Contreras-Saiz E., Solar-Garcia L., Moreno-Gijon M., Suarez-Sanchez A., Diaz-Vico T., Rodicio-Miravalles J.L., Garcia-Gutierrez C., Pila U., Melone S., Martin-Prieto L., Rojo J.A., Gonzalez M., Zorrilla L., Garcia-Marin J.A., Baeza-Murcia M., Pellicer-Franco E., Jimenez-Ballester M.A., Asensio-Gomez L., Gortazar-De-Las-Casas S., Guevara-Martinez J., Ramirez L., Verea S., Anguita F., Navarro G., Criado ADC., Lara M.C., Martinez E.T., Sanchez-Martinez A., Hernandez-Gimenez L., Galofre-Recasens M., Ferrer-Vilela I., Perez-Sanchez L.E., Esteves M.B., Menendez-Moreno A., Baz-Figueroa C., Rosat A., Hontoria M.S., Garcia N.A., Gracia-Roman R., Pascua-Sole M., Pino-Perez O., Garcia-Perez J.M., Pineno-Flores C., Ambrona-Zafra D., Sancho-Muriel J., Alvarez E., Jimenez-Rosellon R., Daga O., Alberca-Paramo A., Sanchez-Garcia S., Garcia-Santos E., Pareja-Ciuro F., Olivares-Oliver C., Navarro-Morales L., Tamayo-Lopez M.J., Tinoco-Gonzalez J., Garcia-Rivera C.O., Agua I.A., Moreno-Suero F., Pereira-Mosquera E., Zerpa C., Llacer E., Diaz A., Caro A., Feliu F., Franco M., Escuder J., Abellan M., Padilla E., Mambrilla-Herrero S., Plua-Muniz K.T., Bailon-Cuadrado M., Tejero-Pintor F.J., Choolani-Bhojwani E., Vila-Zarate C., Delgado-Plasencia L.J., Ponchietti L., Cousins L., Busuttil A., Baird C., Drye N., Brown O.D., Mansour S., Anderson O., Mahapatra R., Clements J.A., D'Souza N., Littlehales D.J., Tang A.M., Byrne B.E., Cunha P., Ogbuokiri C., Eiben P., Gravante G., Kho H., Dobbs S., Doulias T., Ng J., Wilson M., Venugopal R., Wolff J., Akhtar K., Walji H.D., Tognarelli J.M., Knight K.A., Ansari A., Hussaini S.A., Wright E., Brewer H., Rinkoff S., Harries R.L., Fairfield C.J., Abbott T., Jackson A., Wright H.L., Walters U., Carney K., Logan P.C., Mughal Z., Strachan E., Chasty B., Ma J., Mazzeo C., Badii B., Armellini A., Grassia M., Perin A., Ruzzenente A., Magnoli M., Depalma N., Longheu A., Papandrea M., Dova L., De Prizio M., Gusai G.P., Di Zitti L., Geretto P., Azabdaftari A., Chianese G., Elbetti C., Ruffolo C., Giaccari S., Devezas V., Ferreira J.S., Peixoto R., Alshafei A., Simo V., Jose H.S., Ugarte-Sierra B., Salva A.B., Gomez N., Marinello F., Medina-Arana V., Vega L., Ballester M.M., Espina B., Prieto-Nieto M.I., Rodriguez E.C., Padilla-Valverde D., and Duran-Munoz-Cruzado V.M.
Subjects: Adult, humanos, Decision Making, Risk Assessment, NO, apendicectomía, apendicitis, evaluación de riesgos, Appendectomy, Humans, hospital, General, collaborative, LS7_4, right iliac fossa, appendicitis, emergency service, Original Articles, adulto, Appendicitis, adult, appendectomy, humans, risk assessment, decision making, Lower GI, Original Article, appendicitis, prediction models, right iliac fossa pain, Emergency Service, Hospital, toma de decisión
Abstract: Background Appendicitis is the most common general surgical emergency worldwide, but its diagnosis remains challenging. The aim of this study was to determine whether existing risk prediction models can reliably identify patients presenting to hospital in the UK with acute right iliac fossa (RIF) pain who are at low risk of appendicitis. Methods A systematic search was completed to identify all existing appendicitis risk prediction models. Models were validated using UK data from an international prospective cohort study that captured consecutive patients aged 16–45 years presenting to hospital with acute RIF in March to June 2017. The main outcome was best achievable model specificity (proportion of patients who did not have appendicitis correctly classified as low risk) whilst maintaining a failure rate below 5 per cent (proportion of patients identified as low risk who actually had appendicitis). Results Some 5345 patients across 154 UK hospitals were identified, of which two‐thirds (3613 of 5345, 67·6 per cent) were women. Women were more than twice as likely to undergo surgery with removal of a histologically normal appendix (272 of 964, 28·2 per cent) than men (120 of 993, 12·1 per cent) (relative risk 2·33, 95 per cent c.i. 1·92 to 2·84; P, Women in the UK had a disproportionate risk of admission without surgical intervention and had high rates of normal appendicectomy. Risk prediction models to support shared decision‐making were identified by identifying UK adults at low risk of appendicitis. An online calculator is available (http://appy-risk.org). WCC, white cell count; CRP, C‐reactive protein; AIRS, Appendicitis Inflammatory Response Score; AAS, Adult Appendicitis Score. Important differences between men and women
Published: 2019

42. Cross-correlation of DES Y3 lensing and ACT/${\it Planck}$ thermal Sunyaev Zel'dovich Effect II: Modeling and constraints on halo pressure profiles

Author: Pandey, S., Gatti, M., Baxter, E., Hill, J. C., Fang, X., Doux, C., Giannini, G., Raveri, M., DeRose, J., Huang, H., Moser, E., Battaglia, N., Alarcon, A., Amon, A., Becker, M., Campos, A., Chang, C., Chen, R., Choi, A., Eckert, K., Elvin-Poole, J., Everett, S., Ferte, A., Harrison, I., Maccrann, N., Mccullough, J., Myles, J., Alsina, A. Navarro, Prat, J., Rollins, R. P., Sanchez, C., Shin, T., Troxel, M., Tutusaus, I., Yin, B., Aguena, M., Allam, S., Andrade-Oliveira, F., Bernstein, G. M., Bertin, E., Bolliet, B., Bond, J. R., Brooks, D., Calabrese, E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cawthon, R., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Dunkley, J., Evrard, A. E., Ferraro, S., Ferrero, I., Flaugher, B., Fosalba, P., Garcia-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Herner, K., Hincks, A. D., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hughes, J. P., Huterer, D., Jain, B., James, D. J., Jeltema, T., Krause, E., Kuehn, K., Lahav, O., Lima, M., Lokken, M., Madhavacheril, M. S., Maia, M. A. G., Mcmahon, J. J., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Moodley, K., Morgan, R., Nati, F., Niemack, M. D., Page, L., Palmese, A., Paz-Chinchon, F., Pieres, A., Malagon, A. A. Plazas, Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Scarpine, V., Schaan, E., Serrano, S., Sevilla-Noarbe, I., Sheldon, E., Sherwin, B. D., Sifon, C., Smith, M., Soares-Santos, M., Spergel, D., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Varga, T. N., Weller, J., Wollack, E. J., and Xu, Z.
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Astrophysics of Galaxies (astro-ph.GA), FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Hot, ionized gas leaves an imprint on the cosmic microwave background via the thermal Sunyaev Zel'dovich (tSZ) effect. The cross-correlation of gravitational lensing (which traces the projected mass) with the tSZ effect (which traces the projected gas pressure) is a powerful probe of the thermal state of ionized baryons throughout the Universe, and is sensitive to effects such as baryonic feedback. In a companion paper (Gatti et al. 2021), we present tomographic measurements and validation tests of the cross-correlation between galaxy shear measurements from the first three years of observations of the Dark Energy Survey, and tSZ measurements from a combination of Atacama Cosmology Telescope and ${\it Planck}$ observations. In this work, we use the same measurements to constrain models for the pressure profiles of halos across a wide range of halo mass and redshift. We find evidence for reduced pressure in low mass halos, consistent with predictions for the effects of feedback from active galactic nuclei. We infer the hydrostatic mass bias ($B \equiv M_{500c}/M_{\rm SZ}$) from our measurements, finding $B = 1.8\pm0.1$ when adopting the ${\it Planck}$-preferred cosmological parameters. We additionally find that our measurements are consistent with a non-zero redshift evolution of $B$, with the correct sign and sufficient magnitude to explain the mass bias necessary to reconcile cluster count measurements with the ${\it Planck}$-preferred cosmology. Our analysis introduces a model for the impact of intrinsic alignments (IA) of galaxy shapes on the shear-tSZ correlation. We show that IA can have a significant impact on these correlations at current noise levels., 22 pages, 13 figures. Comments welcome
Published: 2021

43. DES Y3 results: Blending shear and redshift biases in image simulations

Author: MacCrann, N., Becker, M. R., McCullough, J., Amon, A., Gruen, D., Jarvis, M., Choi, A., Troxel, M. A., Sheldon, E., Yanny, B., Herner, K., Dodelson, S., Zuntz, J., Eckert, K., Rollins, R. P., Varga, T. N., Bernstein, G. M., Gruendl, R. A., Harrison, I., Hartley, W. G., Sevilla-Noarbe, I., Pieres, A., Bridle, S. L., Myles, J., Alarcon, A., Everett, S., S��nchez, C., Huff, E. M., Tarsitano, F., Gatti, M., Secco, L. F., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Bacon, D., Bertin, E., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Costanzi, M., Crocce, M., Pereira, M. E. S., De Vicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Eifler, T. F., Ferrero, I., Fert��, A., Flaugher, B., Fosalba, P., Frieman, J., Garc��a-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Lahav, O., Lima, M., Maia, M. A. G., March, M., Marshall, J. L., Martini, P., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Muir, J., Ogando, R. L. C., Palmese, A., Paz-Chinch��n, F., Plazas, A. A., Rodriguez-Monroy, M., Roodman, A., Samuroff, S., Sanchez, E., Scarpine, V., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., To, C., Wilkinson, R. D., Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), and DES
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: As the statistical power of galaxy weak lensing reaches percent level precision, large, realistic and robust simulations are required to calibrate observational systematics, especially given the increased importance of object blending as survey depths increase. To capture the coupled effects of blending in both shear and photometric redshift calibration, we define the effective redshift distribution for lensing, $n_{\gamma}(z)$, and describe how to estimate it using image simulations. We use an extensive suite of tailored image simulations to characterize the performance of the shear estimation pipeline applied to the Dark Energy Survey (DES) Year 3 dataset. We describe the multi-band, multi-epoch simulations, and demonstrate their high level of realism through comparisons to the real DES data. We isolate the effects that generate shear calibration biases by running variations on our fiducial simulation, and find that blending-related effects are the dominant contribution to the mean multiplicative bias of approximately $-2\%$. By generating simulations with input shear signals that vary with redshift, we calibrate biases in our estimation of the effective redshfit distribution, and demonstrate the importance of this approach when blending is present. We provide corrected effective redshift distributions that incorporate statistical and systematic uncertainties, ready for use in DES Year 3 weak lensing analyses., Comment: Submitted to MNRAS. See https://www.darkenergysurvey.org/des-year-3-cosmology-results-papers/ for the full DES Y3 cosmology release. Version accepted by mnras
Published: 2021

44. Cross-correlation of DES Y3 lensing and ACT/${\it Planck}$ thermal Sunyaev Zel'dovich Effect I: Measurements, systematics tests, and feedback model constraints

Author: Gatti, M., Pandey, S., Baxter, E., Hill, J. C., Moser, E., Raveri, M., Fang, X., DeRose, J., Giannini, G., Doux, C., Huang, H., Battaglia, N., Alarcon, A., Amon, A., Becker, M., Campos, A., Chang, C., Chen, R., Choi, A., Eckert, K., Elvin-Poole, J., Everett, S., Ferte, A., Harrison, I., Maccrann, N., Mccullough, J., Myles, J., Alsina, A. Navarro, Prat, J., Rollins, R. P., Sanchez, C., Shin, T., Troxel, M., Tutusaus, I., Yin, B., Abbott, T., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bernstein, G., Bertin, E., Bolliet, B., Bond, J. R., Brooks, D., Burke, D. L., Calabrese, E., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cawthon, R., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. da Silva, DeVicente, J., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Dunkley, J., Evrard, A. E., Ferraro, S., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., Garcıa-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Herner, K., Hincks, A. D., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hughes, J. P., Huterer, D., Jain, B., James, D. J., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lidman, C., Lima, M., Lokken, M., Madhavacheril, M. S., Maia, M. A. G., Marshall, J. L., Mcmahon, J. J., Melchior, P., Moodley, K., Mohr, J. J., Morgan, R., Nati, F., Niemack, M. D., Page, L., Palmese, A., Paz-Chinchon, F., Pieres, A., Malagon, A. A. Plazas, Rodriguez-Monroy, M., Romer, A. K., Sanchez, E., Scarpine, V., Schaan, E., Secco, L. F., Serrano, S., Sheldon, E., Sherwin, B. D., Sifon, C., Smith, M., Soares-Santos, M., Spergel, D., Suchyta, E., Tarle, G., Thomas, D., To, C., Tucker, D. L., Varga, T. N., Weller, J., Wilkinson, R. D., Wollack, E. J., and Xu, Z.
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: We present a tomographic measurement of the cross-correlation between thermal Sunyaev-Zeldovich (tSZ) maps from ${\it Planck}$ and the Atacama Cosmology Telescope (ACT) and weak galaxy lensing shears measured during the first three years of observations of the Dark Energy Survey (DES Y3). This correlation is sensitive to the thermal energy in baryons over a wide redshift range, and is therefore a powerful probe of astrophysical feedback. We detect the correlation at a statistical significance of $21\sigma$, the highest significance to date. We examine the tSZ maps for potential contaminants, including cosmic infrared background (CIB) and radio sources, finding that CIB has a substantial impact on our measurements and must be taken into account in our analysis. We use the cross-correlation measurements to test different feedback models. In particular, we model the tSZ using several different pressure profile models calibrated against hydrodynamical simulations. Our analysis marginalises over redshift uncertainties, shear calibration biases, and intrinsic alignment effects. We also marginalise over $\Omega_{\rm m}$ and $\sigma_8$ using ${\it Planck}$ or DES priors. We find that the data prefers the model with a low amplitude of the pressure profile at small scales, compatible with a scenario with strong AGN feedback and ejection of gas from the inner part of the halos. When using a more flexible model for the shear profile, constraints are weaker, and the data cannot discriminate between different baryonic prescriptions., Comment: submitted to PRD
Published: 2021
Full Text: View/download PDF

45. Impact of COVID-19 Pandemic on Cardiovascular Testing in Asia: The IAEA INCAPS-COVID Study

Author: Kudo, T., Lahey, R., Hirschfeld, C.B., Williams, M.C., Lu, B., Alasnag, M., Bhatia, M., Henry Bom, H.-., Dautov, T., Fazel, R., Karthikeyan, G., Keng, F.Y.J., Rubinshtein, R., Better, N., Cerci, R.J., Dorbala, S., Raggi, P., Shaw, L.J., Villines, T.C., Vitola, J.V., Choi, A.D., Malkovskiy, E., Goebel, B., Cohen, Y.A., Randazzo, M., Pascual, T.N.B., Pynda, Y., Dondi, M., Paez, D., Einstein, A.J., Cerci, R., Hinterleitner, G., Lu, Y., Morozova, O., Xu, Z., Cohen, Y., Choi, A., Lopez-Mattei, J., Parwani, P., Nasery, M.N., Goda, A., Shirka, E., Benlabgaa, R., Bouyoucef, S., Medjahedi, A., Nailli, Q., Agolti, M., Aguero, R.N., Alak, M.D.C., Alberguina, L.G., Arronada, G., Astesiano, A., Norton, C.B., Benteo, P., Blanco, J., Bonelli, J.M., Bustos, J.J., Cabrejas, R., Cachero, J., Campisi, R., Canderoli, A., Carames, S., Carrascosa, P., Castro, R., Cendoya, O., Cognigni, L.M., Collaud, C., Cortes, C., Courtis, J., Cragnolino, D., Daicz, M., De La Vega, A., De Maria, S.T., Del Riego, H., Dettori, F., Deviggiano, A., Dragonetti, L., Embon, M., Enriquez, R.E., Ensinas, J., Faccio, F., Facello, A., Garofalo, D., Geronazzo, R., Gonza, N., Gutierrez, L., Guzzo, M.A., Hasbani, V., Huerin, M., Jager, V., Lewkowicz, J.M., Lopez De Munain, M.N.A., Lotti, J.M., Marquez, A., Masoli, O., Masoli, O.H., Mastrovito, E., Mayoraz, M., Melado, G.E., Mele, A., Merani, M.F., Meretta, A.H., Molteni, S., Montecinos, M., Noguera, E., Novoa, C., Sueldo, C.P., Ascani, S.P., Pollono, P., Pujol, M.P., Radzinschi, A., Raimondi, G., Redruello, M., Rodriguez, M., Romero, R.L., Acuna, A.R., Rovaletti, F., San Miguel, L., Solari, L., Strada, B., Traverso, S., Traverzo, S.S., Espeche, M.D.H.V., Weihmuller, J.S., Wolcan, J., Zeffiro, S., Sakanyan, M., Beuzeville, S., Boktor, R., Butler, P., Calcott, J., Carr, L., Chan, V., Chao, C., Chong, W., Dobson, M., Downie, D.A., Dwivedi, G., Elison, B., Engela, J., Francis, R., Gaikwad, A., Basavaraj, A.G., Goodwin, B., Greenough, R., Hamilton-Craig, C., Hsieh, V., Joshi, S., Lederer, K., Lee, K., Lee, J., Magnussen, J., Mai, N., Mander, G., Murton, F., Nandurkar, D., Neill, J., O'Rourke, E., O'Sullivan, P., Pandos, G., Pathmaraj, K., Pitman, A., Poulter, R., Premaratne, M., Prior, D., Ridley, L., Rutherford, N., Salehi, H., Saunders, C., Scarlett, L., Seneviratne, S., Shetty, D., Shrestha, G., Shulman, J., Solanki, V., Stanton, T., Stuart, M., Stubbs, M., Swainson, I., Taubman, K., Taylor, A., Thomas, P., Unger, S., Upton, A., Vamadevan, S., Van Gaal, W., Verjans, J., Voutnis, D., Wayne, V., Wilson, P., Wong, D., Wong, K., Younger, J., Feuchtner, G., Mirzaei, S., Weiss, K., Maroz-Vadalazhskaya, N., Gheysens, O., Homans, F., Moreno-Reyes, R., Pasquet, A., Roelants, V., Van De Heyning, C.M., Rios, R.A., Soldat-Stankovic, V., Stankovic, S., Albernaz Siqueira, M.H., Almeida, A., Alves Togni, P.H., Andrade, J.H., Andrade, L., Anselmi, C., Araujo, R., Azevedo, G., Bezerra, S., Biancardi, R., Grossman, G.B., Brandao, S., Pianta, D.B., Carreira, L., Castro, B., Chang, T., Cunali, F., Cury, R., Dantas, R., de Amorim Fernandes, F., De Lorenzo, A., De Macedo Filho, R., Erthal, F., Fernandes, F., Fernandes, J., De Souza, T.F., Alves, W.F., Ghini, B., Goncalves, L., Gottlieb, I., Hadlich, M., Kameoka, V., Lima, R., Lima, A., Lopes, R.W., Machado e Silva, R., Magalhaes, T., Silva, F.M., Mastrocola, L.E., Medeiros, F., Meneghetti, J.C., Naue, V., Naves, D., Nolasco, R., Nomura, C., Oliveira, J.B., Paixao, E., De Carvalho, F.P., Pinto, I., Possetti, P., Quinta, M., Nogueira Ramos, R.R., Rocha, R., Rodrigues, A., Rodrigues, C., Romantini, L., Sanches, A., Santana, S., Sara da Silva, L., Schvartzman, P., Matushita, C.S., Senra, T., Shiozaki, A., Menezes de Siqueira, M.E., Siqueira, C., Smanio, P., Soares, C.E., Junior, J.S., Bittencourt, M.S., Spiro, B., Mesquita, C.T., Torreao, J., Torres, R., Uellendahl, M., Monte, G.U., Verissimo, O., Cabeda, E.V., Pedras, F.V., Waltrick, R., Zapparoli, M., Naseer, H., Garcheva-Tsacheva, M., Kostadinova, I., Theng, Y., Abikhzer, G., Barette, R., Chow, B., Dabreo, D., Friedrich, M., Garg, R., Hafez, M.N., Johnson, C., Kiess, M., Leipsic, J., Leung, E., Miller, R., Oikonomou, A., Probst, S., Roifman, I., Small, G., Tandon, V., Trivedi, A., White, J., Zukotynski, K., Canessa, J., Munoz, G.C., Concha, C., Hidalgo, P., Lovera, C., Massardo, T., Vargas, L.S., Abad, P., Arturo, H., Ayala, S., Benitez, L., Cadena, A., Caicedo, C., Moncayo, A.C., Gomez, S., Gutierrez Villamil, C.T., Jaimes, C., Londono, J., Londono Blair, J.L., Pabon, L., Pineda, M., Rojas, J.C., Ruiz, D., Escobar, M.V., Vasquez, A., Vergel, D., Zuluaga, A., Gamboa, I.B., Castro, G., Gonzalez, U., Baric, A., Batinic, T., Franceschi, M., Paar, M.H., Jukic, M., Medakovic, P., Persic, V., Prpic, M., Punda, A., Batista, J.F., Gomez Lauchy, J.M., Gutierrez, Y.M., Menendez, R., Peix, A., Rochela, L., Panagidis, C., Petrou, I., Engelmann, V., Kaminek, M., Kincl, V., Lang, O., Simanek, M., Abdulla, J., Bottcher, M., Christensen, M., Gormsen, L.C., Hasbak, P., Hess, S., Holdgaard, P., Johansen, A., Kyhl, K., Norgaard, B.L., Ovrehus, K.A., Ronnow Sand, N.P., Steffensen, R., Thomassen, A., Zerahn, B., Perez, A., Escorza Velez, G.A., Velez, M.S., Abdel Aziz, I.S., Abougabal, M., Ahmed, T., Allam, A., Asfour, A., Hassan, M., Hassan, A., Ibrahim, A., Kaffas, S., Kandeel, A., Ali, M.M., Mansy, A., Maurice, H., Nabil, S., Shaaban, M., Flores, A.C., Poksi, A., Knuuti, J., Kokkonen, V., Larikka, M., Uusitalo, V., Bailly, M., Burg, S., Deux, J.-., Habouzit, V., Hyafil, F., Lairez, O., Proffit, F., Regaieg, H., Sarda-Mantel, L., Tacher, V., Schneider, R.P., Ayetey, H., Angelidis, G., Archontaki, A., Chatziioannou, S., Datseris, I., Fragkaki, C., Georgoulias, P., Koukouraki, S., Koutelou, M., Kyrozi, E., Repasos, E., Stavrou, P., Valsamaki, P., Gonzalez, C., Gutierrez, G., Maldonado, A., Buga, K., Garai, I., Maurovich-Horvat, P., Schmidt, E., Szilveszter, B., Varady, E., Banthia, N., Bhagat, J.K., Bhargava, R., Bhat, V., Choudhury, P., Chowdekar, V.S., Irodi, A., Jain, S., Joseph, E., Kumar, S., Girijanandan Mahapatra, P.D., Mitra, D., Mittal, B.R., Ozair, A., Patel, C., Patel, T., Patel, R., Patel, S., Saxena, S., Sengupta, S., Singh, S., Singh, B., Sood, A., Verma, A., Affandi, E., Alam, P.S., Edison, E., Gunawan, G., Hapkido, H., Hidayat, B., Huda, A., Mukti, A.P., Prawiro, D., Soeriadi, E.A., Syawaluddin, H., Albadr, A., Assadi, M., Emami, F., Houshmand, G., Maleki, M., Rostami, M.T., Zakavi, S.R., Zaid, E.A., Agranovich, S., Arnson, Y., Bar-Shalom, R., Frenkel, A., Knafo, G., Lugassi, R., Maor Moalem, I.S., Mor, M., Muskal, N., Ranser, S., Shalev, A., Albano, D., Alongi, P., Arnone, G., Bagatin, E., Baldari, S., Bauckneht, M., Bertelli, P., Bianco, F., Bonfiglioli, R., Boni, R., Bruno, A., Bruno, I., Busnardo, E., Califaretti, E., Camoni, L., Carnevale, A., Casoni, R., Cavallo, A.U., Cavenaghi, G., Chierichetti, F., Chiocchi, M., Cittanti, C., Colletta, M., Conti, U., Cossu, A., Cuocolo, A., Cuzzocrea, M., De Rimini, M.L., De Vincentis, G., Del Giudice, E., Del Torto, A., Della Tommasina, V., Durmo, R., Erba, P.A., Evangelista, L., Faletti, R., Faragasso, E., Farsad, M., Ferro, P., Florimonte, L., Frantellizzi, V., Fringuelli, F.M., Gatti, M., Gaudiano, A., Gimelli, A., Giubbini, R., Giuffrida, F., Ialuna, S., Laudicella, R., Leccisotti, L., Leva, L., Liga, R., Liguori, C., Longo, G., Maffione, M., Mancini, M.E., Marcassa, C., Milan, E., Nardi, B., Pacella, S., Pepe, G., Pontone, G., Pulizzi, S., Quartuccio, N., Rampin, L., Ricci, F., Rossini, P., Rubini, G., Russo, V., Sacchetti, G.M., Sambuceti, G., Scarano, M., Sciagra, R., Sperandio, M., Stefanelli, A., Ventroni, G., Zoboli, S., Baugh, D., Chambers, D., Madu, E., Nunura, F., Asano, H., Chimura, C.M., Fujimoto, S., Fujisue, K., Fukunaga, T., Fukushima, Y., Fukuyama, K., Hashimoto, J., Ichikawa, Y., Iguchi, N., Imai, M., Inaki, A., Ishimura, H., Isobe, S., Kadokami, T., Kato, T., Kumita, S., Maruno, H., Mataki, H., Miyagawa, M., Morimoto, R., Moroi, M., Nagamachi, S., Nakajima, K., Nakata, T., Nakazato, R., Nanasato, M., Naya, M., Norikane, T., Ohta, Y., Okayama, S., Okizaki, A., Otomi, Y., Otsuka, H., Saito, M., Sakata, S.Y., Sarai, M., Sato, D., Shiraishi, S., Suwa, Y., Takanami, K., Takehana, K., Taki, J., Tamaki, N., Taniguchi, Y., Teragawa, H., Tomizawa, N., Tsujita, K., Umeji, K., Wakabayashi, Y., Yamada, S., Yamazaki, S., Yoneyama, T., Rawashdeh, M., Batyrkhanov, D., Makhdomi, K., Ombati, K., Alkandari, F., Garashi, M., Coie, T.L., Rajvong, S., Kalinin, A., Kalnina, M., Haidar, M., Komiagiene, R., Kviecinskiene, G., Mataciunas, M., Vajauskas, D., Picard, C., Karim, N.K.A., Reichmuth, L., Samuel, A., Allarakha, M.A., Naojee, A.S., Alexanderson-Rosas, E., Barragan, E., Gonzalez-Montecinos, A.B., Cabada, M., Rodriguez, D.C., Carvajal-Juarez, I., Cortes, V., Cortes, F., De La Pena, E., Gama-Moreno, M., Gonzalez, L., Ramirez, N.G., Jimenez-Santos, M., Matos, L., Monroy, E., Morelos, M., Ornelas, M., Ortga Ramirez, J.A., Preciado-Anaya, A., Preciado-Gutierrez, O.U., Barragan, A.P., Rosales Uvera, S.G., Sandoval, S., Tomas, M.S., Sierra-Galan, L.M., Siu, S., Vallejo, E., Valles, M., Faraggi, M., Sereegotov, E., Ilic, S., Ben-Rais, N., Alaoui, N.I., Taleb, S., Pa Myo, K.P., Thu, P.S., Ghimire, R.K., Rajbanshi, B., Barneveld, P., Glaudemans, A., Habets, J., Koopmans, K.P., Manders, J., Pool, S., Scholte, A., Scholtens, A., Slart, R., Thimister, P., Van Asperen, E.-., Veltman, N., Verschure, D., Wagenaar, N., Edmond, J., Ellis, C., Johnson, K., Keenan, R., Kueh, S.H.A., Occleshaw, C., Sasse, A., To, A., Van Pelt, N., Young, C., Cuadra, T., Roque Vanegas, H.B., Soli, I.A., Issoufou, D.M., Ayodele, T., Madu, C., Onimode, Y., Efros-Monsen, E., Forsdahl, S.H., Hildre Dimmen, J.-., Jorgensen, A., Krohn, I., Lovhaugen, P., Braten, A.T., Al Dhuhli, H., Al Kindi, F., Al-Bulushi, N., Jawa, Z., Tag, N., Afzal, M.S., Fatima, S., Younis, M.N., Riaz, M., Saadullah, M., Herrera, Y., Lenturut-Katal, D., Vazquez, M.C., Ortellado, J., Akhter, A., Cao, D., Cheung, S., Dai, X., Gong, L., Han, D., Hou, Y., Li, C., Li, T., Li, D., Li, S., Liu, J., Liu, H., M. Y., N., Sun, K., Tang, G., Wang, J., Wang, X., Wang, Z.-., Wang, Y., Wu, J., Wu, Z., Xia, L., Xiao, J., Xu, L., Yang, Y., Yin, W., Yu, J., Yuan, L., Zhang, T., Zhang, L., Zhang, Y.-., Zhang, X., Zhu, L., Alfaro, A., Abrihan, P., Barroso, A., Cruz, E., Gomez, M.R., Magboo, V.P., Medina, J.M., Obaldo, J., Pastrana, D., Pawhay, C.M., Quinon, A., Tang, J.M., Tecson, B., Uson, K.J., Uy, M., Kostkiewicz, M., Kunikowska, J., Bettencourt, N., Cantinho, G., Ferreira, A., Syed, G., Arnous, S., Atyani, S., Byrne, A., Gleeson, T., Kerins, D., Meehan, C., Murphy, D., Murphy, M., Murray, J., O'Brien, J., Bang, J.-., Bom, H., Cho, S.-., Hong, C.M., Jang, S.J., Jeong, Y.H., Kang, W.J., Kim, J.-., Namgung, C.K., So, Y., Won, K.S., Majstorov, V., Vavlukis, M., Salobir, B.G., Stalc, M., Benedek, T., Benedek, I., Mititelu, R., Stan, C.A., Ansheles, A., Dariy, O., Drozdova, O., Gagarina, N., Gulyaev, V.M., Itskovich, I., Karalkin, A., Kokov, A., Migunova, E., Pospelov, V., Ryzhkova, D., Saifullina, G., Sazonova, S., Sergienko, V., Shurupova, I., Trifonova, T., Ussov, W.Y., Vakhromeeva, M., Valiullina, N., Zavadovsky, K., Zhuravlev, K., Okarvi, S., Saranovic, D.S., Keng, F., Jason See, J.H., Sekar, R., Yew, M.S., Vondrak, A., Bejai, S., Bennie, G., Bester, R., Engelbrecht, G., Evbuomwan, O., Gongxeka, H., Vuuren, M.J., Kaplan, M., Khushica, P., Lakhi, H., Louw, L., Malan, N., Milos, K., Modiselle, M., More, S., Naidoo, M., Scholtz, L., Vangu, M., Aguade-Bruix, S., Blanco, I., Cabrera, A., Camarero, A., Casans-Tormo, I., Cuellar-Calabria, H., Flotats, A., Fuentes Canamero, M.E., Garcia, M.E., Jimenez-Heffernan, A., Leta, R., Diaz, J.L., Lumbreras, L., Marquez-Cabeza, J.J., Martin, F., Martinez de Alegria, A., Medina, F., Canal, M.P., Peiro, V., Pubul-Nunez, V., Rayo Madrid, J.I., Rey, C.R., Perez, R.R., Ruiz, J., Hernandez, G.S., Sevilla, A., Zeidan, N., Nanayakkara, D., Udugama, C., Simonsson, M., Alkadhi, H., Buechel, R.R., Burger, P., Ceriani, L., De Boeck, B., Grani, C., Juillet de Saint Lager Lucas, A., Kamani, C.H., Kawel-Boehm, N., Manka, R., Prior, J.O., Rominger, A., Vallee, J.-., Khiewvan, B., Premprabha, T., Thientunyakit, T., Sellem, A., Kir, K.M., Sayman, H., Sebikali, M.J., Muyinda, Z., Kmetyuk, Y., Korol, P., Mykhalchenko, O., Pliatsek, V., Satyr, M., Albalooshi, B., Ahmed Hassan, M.I., Anderson, J., Bedi, P., Biggans, T., Bularga, A., Bull, R., Burgul, R., Carpenter, J.-., Coles, D., Cusack, D., Deshpande, A., Dougan, J., Fairbairn, T., Farrugia, A., Gopalan, D., Gummow, A., Ramkumar, P.G., Hamilton, M., Harbinson, M., Hartley, T., Hudson, B., Joshi, N., Kay, M., Kelion, A., Khokhar, A., Kitt, J., Low, C., Mak, S.M., Marousa, N., Martin, J., Mcalindon, E., Menezes, L., Morgan-Hughes, G., Moss, A., Murray, A., Nicol, E., Patel, D., Peebles, C., Pugliese, F., Luis Rodrigues, J.C., Rofe, C., Sabharwal, N., Schofield, R., Semple, T., Sharma, N., Strouhal, P., Subedi, D., Topping, W., Tweed, K., Weir-Mccall, J., Abbara, S., Abbasi, T., Abbott, B., Abohashem, S., Abramson, S., Al-Abboud, T., Al-Mallah, M., Almousalli, O., Ananthasubramaniam, K., Kumar, M.A., Askew, J., Attanasio, L., Balmer-Swain, M., Bayer, R.R., Bernheim, A., Bhatti, S., Bieging, E., Blankstein, R., Bloom, S., Blue, S., Bluemke, D., Borges, A., Branch, K., Bravo, P., Brothers, J., Budoff, M., Bullock-Palmer, R., Burandt, A., Burke, F.W., Bush, K., Candela, C., Capasso, E., Cavalcante, J., Chang, D., Chatterjee, S., Chatzizisis, Y., Cheezum, M., Chen, T., Chen, J., Chen, M., Clarcq, J., Cordero, A., Crim, M., Danciu, S., Decter, B., Dhruva, N., Doherty, N., Doukky, R., Dunbar, A., Duvall, W., Edwards, R., Esquitin, K., Farah, H., Fentanes, E., Ferencik, M., Fisher, D., Fitzpatrick, D., Foster, C., Fuisz, T., Gannon, M., Gastner, L., Gerson, M., Ghoshhajra, B., Goldberg, A., Goldner, B., Gonzalez, J., Gore, R., Gracia-Lopez, S., Hage, F., Haider, A., Haider, S., Hamirani, Y., Hassen, K., Hatfield, M., Hawkins, C., Hawthorne, K., Heath, N., Hendel, R., Hernandez, P., Hill, G., Horgan, S., Huffman, J., Hurwitz, L., Iskandrian, A., Janardhanan, R., Jellis, C., Jerome, S., Kalra, D., Kaviratne, S., Kay, F., Kelly, F., Khalique, O., Kinkhabwala, M., Iii, G.K., Kircher, J., Kirkbride, R., Kontos, M., Kottam, A., Krepp, J., Layer, J., Lee, S.H., Leppo, J., Lesser, J., Leung, S., Lewin, H., Litmanovich, D., Liu, Y., Magurany, K., Markowitz, J., Marn, A., Matis, S.E., Mckenna, M., Mcrae, T., Mendoza, F., Merhige, M., Min, D., Moffitt, C., Moncher, K., Moore, W., Morayati, S., Morris, M., Mossa-Basha, M., Mrsic, Z., Murthy, V., Nagpal, P., Napier, K., Nelson, K., Nijjar, P., Osman, M., Passen, E., Patel, A., Patil, P., Paul, R., Phillips, L., Polsani, V., Poludasu, R., Pomerantz, B., Porter, T., Prentice, R., Pursnani, A., Rabbat, M., Ramamurti, S., Rich, F., Luna, H.R., Robinson, A., Robles, K., Rodriguez, C., Rorie, M., Rumberger, J., Russell, R., Sabra, P., Sadler, D., Schemmer, M., Schoepf, U.J., Shah, S., Shah, N., Shanbhag, S., Sharma, G., Shayani, S., Shirani, J., Shivaram, P., Sigman, S., Simon, M., Slim, A., Smith, D., Smith, A., Soman, P., Srichai-Parsia, M.B., Streeter, J., T, A., Tawakol, A., Thomas, D., Thompson, R., Torbet, T., Trinidad, D., Ullery, S., Unzek, S., Uretsky, S., Vallurupalli, S., Verma, V., Waller, A., Wang, E., Ward, P., Weissman, G., Wesbey, G., White, K., Winchester, D., Wolinsky, D., Yost, S., Zgaljardic, M., Alonso, O., Beretta, M., Ferrando, R., Kapitan, M., Mut, F., Djuraev, O., Rozikhodjaeva, G., Le Ngoc, H., Mai, S.H., and Nguyen, X.C.
Subjects: INCAPS COVID Investigators Group, Pediatric Research Initiative, positron emission tomography, CTA, SARS-CoV-2, cardiac testing, invasive coronary angiography, Prevention, coronavirus, coronavirus disease-19, COVID-19, global health, Settore MED/11 - Malattie dell'Apparato Cardiovascolare, cardiac magnetic resonance, cardiovascular disease, NO, transthoracic echocardiography, PET, Good Health and Well Being, severe acute respiratory syndrome-coronavirus-2, TTE, ICA, CMR, computed tomographic angiography
Abstract: BackgroundThe coronavirus disease-2019 (COVID-19) pandemic significantly affected management of cardiovascular disease around the world. The effect of the pandemic on volume of cardiovascular diagnostic procedures is not known.ObjectivesThis study sought to evaluate the effects of the early phase of the COVID-19 pandemic on cardiovascular diagnostic procedures and safety practices in Asia.MethodsThe International Atomic Energy Agency conducted a worldwide survey to assess changes in cardiovascular procedure volume and safety practices caused by COVID-19. Testing volumes were reported for March 2020 and April 2020 and were compared to those from March 2019. Data from 180 centers across 33 Asian countries were grouped into 4 subregions for comparison.ResultsProcedure volumes decreased by 47% from March 2019 to March 2020, showing recovery from March 2020 to April 2020 in Eastern Asia, particularly in China. The majority of centers cancelled outpatient activities and increased time per study. Practice changes included implementing physical distancing and restricting visitors. Although COVID testing was not commonly performed, it was conducted in one-third of facilities in Eastern Asia. The most severe reductions in procedure volumes were observed in lower-income countries, where volumes decreased 81% from March 2019 to April2020.ConclusionsThe COVID-19 pandemic in Asia caused significant reductions in cardiovascular diagnostic procedures, particularly in low-income countries. Further studies on effects of COVID-19 on cardiovascular outcomes and changes in care delivery are warranted.
Published: 2021

46. Dark energy survey year 3 results: Weak lensing shape catalogue

Author: Gatti, M., Tutusaus, Isaac, Castander, Francisco J., Crocce, Martín, García-Bellido, Juan, Serrano, S., Wilkinson, Reese D., DES Collaboration, National Science Foundation (US), Ministerio de Economía y Competitividad (España), European Commission, and Instituto Nacional de Ciência e Tecnologia (Brasil)
Subjects: image processing [Techniques], Surveys, weak [Gravitational lensing], data analysis [Methods], Catalogues, observations [Cosmology]
Abstract: Gatti, M., et al. (DES Collaboration) We present and characterize the galaxy shape catalogue from the first 3 yr of Dark Energy Survey (DES) observations, over an effective area of 4143 deg2 of the southern sky. We describe our data analysis process and our self-calibrating shear measurement pipeline metacalibration, which builds and improves upon the pipeline used in the DES Year 1 analysis in several aspects. The DES Year 3 weak-lensing shape catalogue consists of 100 204 026 galaxies, measured in the riz bands, resulting in a weighted source number density of neff = 5.59 gal arcmin-2 and corresponding shape noise σe = 0.261. We perform a battery of internal null tests on the catalogue, including tests on systematics related to the point spread function (PSF) modelling, spurious catalogue B-mode signals, catalogue contamination, and galaxy properties. Based in part on observations at Cerro Tololo Inter-American Observatory at NSF’s NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under grants AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MINECO under grants AYA2015-71825, ESP2015-66861, FPA2015-68048, SEV-2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA programme of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Program (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) e-Universe (CNPq grant 465376/2014-2).
Published: 2021

47. DeepZipper: A Novel Deep Learning Architecture for Lensed Supernovae Identification

Author: Morgan, R, Nord, B, Bechtol, K, González, SJ, Buckley-Geer, E, Möller, A, Park, JW, Kim, AG, Birrer, S, Aguena, M, Annis, J, Bocquet, S, Brooks, D, Carnero Rosell, A, Carrasco Kind, M, Carretero, J, Cawthon, R, Da Costa, LN, Davis, TM, De Vicente, J, Doel, P, Ferrero, I, Friedel, D, Frieman, J, García-Bellido, J, Gatti, M, Gaztanaga, E, Giannini, G, Gruen, D, Gruendl, RA, Gutierrez, G, Hollowood, DL, Honscheid, K, James, DJ, Kuehn, K, Kuropatkin, N, Maia, MAG, Miquel, R, Palmese, A, Paz-Chinchón, F, Pereira, MES, Pieres, A, Plazas Malagón, AA, Reil, K, Roodman, A, Sanchez, E, Smith, M, Suchyta, E, Swanson, MEC, Tarle, G, To, C, National Science Foundation (US), Agencia Estatal de Investigación (España), Ministerio de Ciencia, Innovación y Universidades (España), Generalitat de Catalunya, European Commission, European Research Council, Ministerio de Economía y Competitividad (España), UAM. Departamento de Física Teórica, Morgan, R [0000-0002-7016-5471], Nord, B [0000-0001-6706-8972], Bechtol, K [0000-0001-8156-0429], González, SJ [0000-0001-7282-3864], Buckley-Geer, E [0000-0002-3304-0733], Möller, A [0000-0001-8211-8608], Park, JW [0000-0002-0692-1092], Birrer, S [0000-0003-3195-5507], Aguena, M [0000-0001-5679-6747], Annis, J [0000-0002-0609-3987], Bocquet, S [0000-0002-4900-805X], Brooks, D [0000-0002-8458-5047], Carnero Rosell, A [0000-0003-3044-5150], Carrasco Kind, M [0000-0002-4802-3194], Carretero, J [0000-0002-3130-0204], Cawthon, R [0000-0003-2965-6786], Da Costa, LN [0000-0002-7731-277X], Davis, TM [0000-0002-4213-8783], De Vicente, J [0000-0001-8318-6813], Friedel, D [0000-0002-3632-7668], Frieman, J [0000-0003-4079-3263], García-Bellido, J [0000-0002-9370-8360], Gaztanaga, E [0000-0001-9632-0815], Giannini, G [0000-0002-3730-1750], Gruen, D [0000-0003-3270-7644], Gruendl, RA [0000-0002-4588-6517], Gutierrez, G [0000-0003-0825-0517], Hollowood, DL [0000-0002-9369-4157], Honscheid, K [0000-0002-6550-2023], James, DJ [0000-0001-5160-4486], Kuehn, K [0000-0003-0120-0808], Kuropatkin, N [0000-0003-2511-0946], Maia, MAG [0000-0001-9856-9307], Miquel, R [0000-0002-6610-4836], Palmese, A [0000-0002-6011-0530], Paz-Chinchón, F [0000-0003-1339-2683], Pieres, A [0000-0001-9186-6042], Plazas Malagón, AA [0000-0002-2598-0514], Roodman, A [0000-0001-5326-3486], Sanchez, E [0000-0002-9646-8198], Smith, M [0000-0002-3321-1432], Suchyta, E [0000-0002-7047-9358], Tarle, G [0000-0003-1704-0781], To, C [0000-0001-7836-2261], and Apollo - University of Cambridge Repository
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Física, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Galaxies, Lens, Space and Planetary Science, astro-ph.CO, Astrophysics - Instrumentation and Methods for Astrophysics, Quasars, Instrumentation and Methods for Astrophysics (astro-ph.IM), astro-ph.IM, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract: Morgan et al., Large-scale astronomical surveys have the potential to capture data on large numbers of strongly gravitationally lensed supernovae (LSNe). To facilitate timely analysis and spectroscopic follow-up before the supernova fades, an LSN needs to be identified soon after it begins. To quickly identify LSNe in optical survey data sets, we designed ZipperNet, a multibranch deep neural network that combines convolutional layers (traditionally used for images) with long short-term memory layers (traditionally used for time series). We tested ZipperNet on the task of classifying objects from four categories—no lens, galaxy-galaxy lens, lensed Type-Ia supernova, lensed core-collapse supernova—within high-fidelity simulations of three cosmic survey data sets: the Dark Energy Survey, Rubin Observatory's Legacy Survey of Space and Time (LSST), and a Dark Energy Spectroscopic Instrument (DESI) imaging survey. Among our results, we find that for the LSST-like data set, ZipperNet classifies LSNe with a receiver operating characteristic area under the curve of 0.97, predicts the spectroscopic type of the lensed supernovae with 79% accuracy, and demonstrates similarly high performance for LSNe 1–2 epochs after first detection. We anticipate that a model like ZipperNet, which simultaneously incorporates spatial and temporal information, can play a significant role in the rapid identification of lensed transient systems in cosmic survey experiments., R. Morgan thanks the Universities Research Association Fermilab Visiting Scholars Program for funding his work on this project. R. Morgan also thanks the LSSTC Data Science Fellowship Program, which is funded by LSSTC, NSF Cybertraining grant #1829740, the Brinson Foundation, and the Moore Foundation; his participation in the program has benefited this work. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship Program under grant No. 1744555. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship Program under grant No. 1744555. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenössische Technische Hochschule (ETH) Zürich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Ciències de l'Espai (IEEC/CSIC), the Institut de Física d'Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universität München and the associated Excellence Cluster Universe, the University of Michigan, NSF's NOIRLab, the University of Nottingham, The Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex, Texas A&M University, and the OzDES Membership Consortium. Based in part on observations at Cerro Tololo Inter-American Observatory at NSF's NOIRLab (NOIRLab Prop. ID 2012B-0001; PI: J. Frieman), which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. The DES data management system is supported by the National Science Foundation under grant Numbers AST-1138766 and AST-1536171. The DES participants from Spanish institutions are partially supported by MICINN under grants ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, and MDM-2015-0509, some of which include ERDF funds from the European Union. IFAE is partially funded by the CERCA program of the Generalitat de Catalunya. Research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Program (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciência e Tecnologia (INCT) e-Universe (CNPq grant 465376/2014-2).
Published: 2021
Full Text: View/download PDF

48. Two-dimensional and three-dimensional cardiac magnetic resonance feature-tracking myocardial strain analysis in acute myocarditis patients with preserved ejection fraction

Author: Gatti M., Palmisano A., Faletti R., Benedetti G., Bergamasco L., Bioletto F., Peretto G., Sala S., De Cobelli F., Fonio P., Esposito A., PALMISANO , ANNA, Gatti, M., Palmisano, A., Faletti, R., Benedetti, G., Bergamasco, L., Bioletto, F., Peretto, G., Sala, S., De Cobelli, F., Fonio, P., and Esposito, A.
Subjects: Male, Myocarditi, Left, Predictive Value of Test, 030204 cardiovascular system & hematology, Ventricular Function, Left, Imaging, 030218 nuclear medicine & medical imaging, Ventricular Dysfunction, Left, Computer-Assisted, 0302 clinical medicine, Acute myocarditi, Ventricular Dysfunction, Ventricular Function, Prospective Studies, Cardiac imaging, Ejection fraction, Middle Aged, Magnetic Resonance Imaging, Myocarditis, Italy, Cine, Acute myocarditis, Acute Disease, Cardiology, Diastolic dysfunction, Female, Case-Control Studie, Cardiology and Cardiovascular Medicine, Human, Adult, medicine.medical_specialty, Diastole, Magnetic Resonance Imaging, Cine, Myocardial strain analysi, 03 medical and health sciences, Young Adult, Imaging, Three-Dimensional, Predictive Value of Tests, Internal medicine, Image Interpretation, Computer-Assisted, medicine, Humans, Radiology, Nuclear Medicine and imaging, Image Interpretation, Myocardial strain analysis, business.industry, Cardiovascular magnetic resonance, Feature tracking, Case-Control Studies, Myocardial Contraction, Stroke Volume, medicine.disease, Prospective Studie, Three-Dimensional, Myocardial strain, Cardiac magnetic resonance, business
Abstract: To explore the potential role of two- (2D) and three-dimensional (3D) cardiac magnetic resonance (CMR) feature tracking (FT) myocardial strain analysis in identifying sub-clinical myocardial systolic and diastolic dysfunction in acute myocarditis patients with preserved ejection fraction (EF). Prospective two centre study-control study. Thirty patients (9 female, 37.2 ± 11.8years.) with a CMR diagnosis of acute myocarditis according to the Lake Louise Criteria and preserved EF (≥ 55%) were included in the analysis. CMR data from 24 healthy volunteers (11 female, 36.2 ± 12.5years.) served as control. 2D and 3D LV tissue tracking analysis were performed in a random fashion by two double-blinded operators. Variables were checked for normality and analysed with parametric test. The baseline characteristics of myocarditis patients with preserved EF and the healthy volunteers were perfectly comparable, except for the LV mass index and T1 and T2 mapping values (p < 0.001). The results of the interobserver variability in the 2D and 3D LV CMR FT myocardial strain analysis were p > 0.42, ICC > 0.80 and η 2 > 0.98. There was no statistical difference in 2D and 3D global radial, circumferential and longitudinal strain peak (%) and both systolic and diastolic strain rate (1/s) between acute myocarditis with preserved EF and healthy volunteers (all p = ns). There were no difference in 2D and 3D global radial, circumferential and longitudinal strain peak and both systolic and diastolic strain rate of the LV between acute myocarditis patients with preserved ejection fraction and healthy volunteers.
Published: 2019

49. Sistema socio-assistenziale e volontariato in Spagna e in Italia: percorsi evolutivi e contesto istituzionale

Author: Accorinti M. Gatti M.
Subjects: Sistema di welfare spagnolo, Terzo settore, Volontariato, Riforme
Abstract: Il testo approfondisce il sistema di welfare spagnolo con un approccio di tipo storico-evolutivo e i nuovi processi di riforma del Terzo settore e del volontariato. È la promulgazione della Costitució del 1978, infatti, ad aver permesso lo sviluppo molto più coordinato e organizzato dell'azione volontaria. Partendo da un'analisi storica e comparativa, il saggio esamina anche l'attuale legislazione spagnola sul volontariato, comparandola con quella italiana in materia, allo scopo di sottolineare le analogie e le differenze tra i due paesi.
Published: 2020

50. Identification of the hydantoin alkaloids parazoanthines as novel CXCR4 antagonists by computational and in vitro functional characterization

Author: Vitale, R.M. Thellung, S. Tinto, F. Solari, A. Gatti, M. Nuzzo, G. Ioannou, E. Roussis, V. Ciavatta, M.L. Manzo, E. Florio, T. Amodeo, P.
Abstract: CXCR4 chemokine receptor represents an attractive pharmacological target due to its key role in cancer metastasis and inflammatory diseases. Starting from our previously-developed pharmacophoric model, we applied a combined computational and experimental approach that led to the identification of the hydantoin alkaloids parazoanthines, isolated from the Mediterranean Sea anemone Parazoanthus axinellae, as novel CXCR4 antagonists. Parazoanthine analogues were then synthesized to evaluate the contribution of functional groups to the overall activity. Within the panel of synthesized natural and non-natural parazoanthines, parazoanthine-B was identified as the most potent CXCR4 antagonist with an IC50 value of 9.3 nM, even though all the investigated compounds were able to antagonize in vitro the down-stream effects of CXC12, albeit with variable potency and efficacy. The results of our study strongly support this class of small molecules as potent CXCR4 antagonists in tumoral pathologies characterized by an overexpression of this receptor. Furthermore, their structure–activity relationships allowed the optimization of our pharmacophoric model, useful for large-scale in silico screening. © 2020 Elsevier Inc.
Published: 2020

Catalog

Books, media, physical & digital resources

See catalog results

Searchworks

Select search scope, currently: Articles Catalog books, media & more in Jio Institute collections Articles journal articles & other e-resources

Search

Search Constraints

Refine your results

Search Limiters

Topic

Publication Year Range

Language

Journal

Database

Publisher

389 results on '"Gatti M."'

Search Results

Catalog

Select search scope, currently: Articles

Catalog

books, media & more in Jio Institute collections

Articles

journal articles & other e-resources