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2,193 results on '"Juan Garcia"'

401. C/2014 UN271(Bernardinelli-Bernstein): The Nearly Spherical Cow of Comets

Author

David J. James, R. Cawthon, H. T. Diehl, Maria E. S. Pereira, Josh Frieman, Ramon Miquel, Y.-H. Zhang, David J. Brooks, D. L. Hollowood, S. Serrano, Enrique Gaztanaga, Benjamin T. Montet, Marcelle Soares-Santos, Robert Weryk, A. Carnero Rosell, G. Tarle, R. L. C. Ogando, E. Bertin, Juan Garcia-Bellido, I. Ferrero, M. Costanzi, J. Carretero, Chun-Hao To, E. J. Sanchez, A. Roodman, Richard J. Wainscoat, A. A. Plazas Malagón, J. Gschwend, Adriano Pieres, M. A. G. Maia, M. Rodriguez-Monroy, Salcedo Romero de Ávila, A. R. Walker, M. Carrasco Kind, B. Flaugher, Gary Bernstein, Samuel Hinton, Robert Morgan, S. Everett, M. N. K. Smith, F. Andrade-Oliveira, G. Gutierrez, J. De Vicente, A. K. Romer, Pedro H. Bernardinelli, K. Kuehn, Michael Troxel, E. Suchyta, Jennifer L. Marshall, J. Annis, Michael Schubnell, O. Lahav, D. L. Burke, S. Allam, Robert A. Gruendl, C. J. Conselice, Michel Aguena, I. Sevilla-Noarbe, N. Kuropatkin, T. N. Varga, L. N. da Costa, Felipe Menanteau, K. Honscheid, M. E. C. Swanson, F. Paz-Chinchón, Daniel Gruen, D. W. Gerdes, National Science Foundation (US), Ministerio de Ciencia, Innovación y Universidades (España), Generalitat de Catalunya, European Commission, Instituto Nacional de Ciência e Tecnologia (Brasil), UAM. Departamento de Física Teórica, University of Pennsylvania, University of New South Wales, University of Western Ontario, University of Hawaii, Laboratório Interinstitucional de E-Astronomia - LIneA, Fermi National Accelerator Laboratory, Universidade Estadual Paulista (UNESP), Universidad Autonoma de Madrid, Institut d'Astrophysique de Paris, University College London, Stanford University, SLAC National Accelerator Laboratory, National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign, Barcelona Institute of Science and Technology, University of Wisconsin-Madison, University of Manchester, School of Physics and Astronomy, University of Trieste, INAF-Osservatorio Astronomico di Trieste, Institute for Fundamental Physics of the Universe, Observatório Nacional, University of Michigan, Universitat Hamburg, Medioambientales y Tecnológicas (CIEMAT), Santa Cruz Institute for Particle Physics, University of Oslo, University of Chicago, Institut d'Estudis Espacials de Catalunya (IEEC), Institute of Space Sciences (ICE CSIC), Ludwig-Maximilians-Universitat, University of Queensland, Ohio State University, Center for Astrophysics | Harvard and Smithsonian, Macquarie University, Lowell Observatory, Texas A and M University, Institució Catalana de Recerca i Estudis Avancats, University of Cambridge, Peyton Hall, University of Sussex, University of Southampton, Oak Ridge National Laboratory, 382 Via Pueblo Mall, Duke University, Max Planck Institute for Extraterrestrial Physics, Ludwig-Maximilians Universitat München, NSF's National Optical-Infrared Astronomy Research Laboratory, Bernardinelli, P. H., Bernstein, G. M., Montet, B. T., Weryk, R., Wainscoat, R., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Avila, S., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Kind, M. C., Carretero, J., Cawthon, R., Conselice, C., Costanzi, M., Da Costa, L. N., Pereira, M. E. S., De Vicente, J., Diehl, H. T., Everett, S., Ferrero, I., Flaugher, B., Frieman, J., Garcia-Bellido, J., 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., Lahav, O., Maia, M. A. G., Marshall, J. L., Menanteau, F., Miquel, R., Morgan, R., Ogando, R. L. C., Paz-Chinchon, F., Pieres, A., Malagon, A. A. P., Rodriguez-Monroy, M., Romer, A. K., Roodman, A., Sanchez, E., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., To, C., Troxel, M. A., Varga, T. N., Walker, A. R., and Zhang, Y.

Subjects
Rotation period, Absolute magnitude, Brightness, Long period comets, Small Solar System bodies, Comet nuclei, Comet dynamics, Comet origins, 933, 1469, 2160, 2213, 2203, Astrophysics - Earth and Planetary Astrophysics, Comet, FOS: Physical sciences, Astrophysics, 01 natural sciences, Comet origin, Long Period Comets (933), Geometric albedo, 0103 physical sciences, Comet Nuclei (2160), Surface brightness, 010303 astronomy & astrophysics, Earth and Planetary Astrophysics (astro-ph.EP), Physics, Long period comet, Small Solar System Bodies (1469), 05 social sciences, Uranus, 050301 education, Física, Astronomy and Astrophysics, Comet dynamic, Radiative equilibrium, Small Solar System bodie, Comet Dynamics (2213), Comet Origins (2203), Space and Planetary Science, 0503 education
Abstract

Comet C/2014 UN271 (Bernardinelli-Bernstein), incoming from the Oort cloud, is remarkable in having the brightest (and presumably largest) nucleus of any well-measured comet and having been discovered at the heliocentric distance r h ≈ 29 au, farther than any Oort cloud comet. In this work, we describe the discovery process and observations and the properties that can be inferred from images recorded until the first reports of activity in 2021 June. The orbit has i = 95°, with a perihelion of 10.97 au to be reached in 2031 and a previous aphelion at 40,400 ± 260 au. Backward integration of the orbit under a standard Galactic tidal model and known stellar encounters suggests a perihelion of q ≈ 18 au on its previous perihelion passage 3.5 Myr ago; hence, the current data could be the first ever obtained of a comet that has not been inside Uranus's orbit in 4 Gyr. The photometric data show an unresolved nucleus with absolute magnitude H r = 8.0, colors that are typical of comet nuclei or Damocloids, and no secular trend as it traversed the range 34-23 au. For the r-band geometric albedo p r , this implies a diameter of km. There is strong evidence of brightness fluctuations at the ±0.2 mag level, but no rotation period can be discerned. A coma, nominally consistent with a "stationary"1/ρ surface brightness distribution, grew in scattering cross section at an exponential rate from A f ρ ≈ 1 to ≈150 m as the comet approached from 28 to 20 au. The activity rate is consistent with a very simple model of sublimation of a surface species in radiative equilibrium with the Sun. The inferred enthalpy of sublimation matches those of CO2 and NH3. More volatile species, such as N2, CH4, and CO, must be far less abundant on the sublimating surfaces., 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
2021

402. The Clustering Dynamics of Primordial Black Boles in N-Body Simulations

Author

Juan Garcia-Bellido, Manuel Trashorras, Savvas Nesseris, UAM.Departamento de Física Teórica, Instituto de Física Teórica (IFT), Ministerio de Economía y Competitividad (España), and Ministerio de Ciencia, Innovación y Universidades (España)

Subjects
lcsh:QC793-793.5, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Stellar mass, Dark matter, Black Hole Mergers, FOS: Physical sciences, General Physics and Astronomy, Binary number, Primordial black hole, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, General Relativity and Quantum Cosmology, dark matter, 0103 physical sciences, Primordial Black Holes, Cluster (physics), Mass segregation, Dark Matter, N-body simulations, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, black hole mergers, Physics, 010308 nuclear & particles physics, lcsh:Elementary particle physics, primordial black holes, Física, N-Body Simulations, Astronomía, black hole binaries, Black Hole Binaries, Halo, Phenomenology (particle physics), Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

© 2021 by the authors., We explore the possibility that Dark Matter (DM) may be explained by a nonuniform background of approximately stellar mass clusters of Primordial Black Holes (PBHs) by simulating the evolution from recombination to the present with over 5000 realisations using a Newtonian N-body code. We compute the cluster rate of evaporation and extract the binary and merged sub-populations along with their parent and merger tree histories, lifetimes and formation rates, the dynamical and orbital parameter profiles, the degree of mass segregation and dynamical friction and power spectrum of close encounters. Overall, we find that PBHs can constitute a viable DM candidate, and that their clustering presents a rich phenomenology throughout the history of the Universe. We show that binary systems constitute about 9.5% of all PBHs at present, with mass ratios of q¯B=0.154, and total masses of m¯T,B=303M⊙. Merged PBHs are rare, about 0.0023% of all PBHs at present, with mass ratios of q¯B=0.965 with total and chirp masses of m¯T,B=1670M⊙ and m¯c,M=642M⊙, respectively. We find that cluster puffing up and evaporation leads to bubbles of these PBHs of order 1 kpc containing at present times about 36% of objects and mass, with one-hundred pc-sized cores. We also find that these PBH sub-haloes are distributed in wider PBH haloes of order hundreds of kpc, containing about 63% of objects and mass, coinciding with the sizes of galactic halos. We find at last high rates of close encounters of massive Black Holes (M∼1000M⊙), with ΓS=(1.2+5.9−0.9)×107yr−1Gpc−3 and mergers with ΓM=1337±41yr−1Gpc−3., This research was funded by Research Project PGC2018-094773-B-C32 [MINECO-FEDER]; Centro de Excelencia Severo Ochoa Program SEV-2016-0597; Ramón y Cajal program through Grant No. RYC-2014-15843; Grant No. BES-2016-077817 (MINECO-FPI).

Published
2021

403. Galaxy morphological classification catalogue of the Dark Energy Survey Year 3 data with convolutional neural networks

Author

G. Tarle, M. Carrasco Kind, F. Andrade-Oliveira, Kyler Kuehn, D. L. Burke, Josh Frieman, I. Sevilla-Noarbe, M. Soares-Santos, H. T. Diehl, N. Kuropatkin, Ting-Yun Cheng, Daniel Thomas, Alfonso Aragón-Salamanca, A. Choi, S. Allam, Robert A. Gruendl, S. Everett, Alex Drlica-Wagner, K. D. Eckert, L. N. da Costa, K. Honscheid, J. Carretero, F. Paz-Chinchón, E. J. Sanchez, David J. Brooks, Samuel Hinton, Juan Garcia-Bellido, Maria E. S. Pereira, David J. James, D. L. Hollowood, Asa F. L. Bluck, S. Serrano, Pablo Fosalba, G. Gutierrez, M. Smith, J. Annis, A. A. Plazas Malagón, M. A. G. Maia, A. Roodman, Tommaso Giannantonio, Adriano Pieres, Daniel Gruen, M. E. C. Swanson, C To, V. Scarpine, Elisabeth Krause, E. Suchyta, August E. Evrard, D. W. Gerdes, Michel Aguena, Felipe Menanteau, I. Ferrero, M. Costanzi, Ramon Miquel, J. De Vicente, J. Gschwend, Christopher J. Conselice, M. March, Ofer Lahav, Robert Morgan, National Science Foundation (US), Ministerio de Economía y Competitividad (España), European Commission, Australian Research Council, Durham University, University Park, University of Manchester, Universidade de São Paulo (USP), Laboratório Interinstitucional de e-Astronomia – LIneA, Fermi National Accelerator Laboratory, Universidade Estadual Paulista (UNESP), University of Cambridge, University College London, Stanford University, SLAC National Accelerator Laboratory, National Center for Supercomputing Applications, University of Illinois at Urbana–Champaign, Barcelona Institute of Science and Technology, Ohio State University, University of Trieste, INAF – Osservatorio Astronomico di Trieste, Institute for Fundamental Physics of the Universe, Observatório Nacional, University of Michigan, Medioambientales y Tecnológicas (CIEMAT), University of Chicago, University of Pennsylvania, Santa Cruz Institute for Particle Physics, University of Oslo, Institut d’Estudis Espacials de Catalunya (IEEC), CSIC), Universidad Autonoma de Madrid, University of Queensland, Harvard & Smithsonian, University of Arizona, Macquarie University, Lowell Observatory, Institució Catalana de Recerca i Estudis Avançats, University of Wisconsin–Madison, Peyton Hall, University of Southampton, Oak Ridge National Laboratory, University of Portsmouth, Cheng, Ting-Yun, Conselice, Christopher J., Aragón-Salamanca, Alfonso, Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bluck, A. F. L., Brooks, D., Burke, D. L., Carrasco Kind, M., Carretero, J., Choi, A., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Diehl, H. T., Drlica-Wagner, A., Eckert, K., Everett, S., Evrard, A. E., Ferrero, I., Fosalba, P., Frieman, J., García-Bellido, J., Gerdes, D. W., Giannantonio, T., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Maia, M. A. G., March, M., Menanteau, F., Miquel, R., Morgan, R., Paz-Chinchón, F., Pieres, A., Plazas Malagón, A. A., Roodman, A., Sanchez, E., Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Thomas, D., and To, C.

Subjects
structure [Galaxies], FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Disc galaxy, 01 natural sciences, Convolutional neural network, Methods: observational, Methods: data analysis, Galaxies: structure, 0103 physical sciences, observational [Methods], 10. No inequality, data analysis [Methods], 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, methods: observational, methods: data analysis, catalogues, galaxies: structure, Astrophysics - Astrophysics of Galaxies, Physics, 010308 nuclear & particles physics, Astronomy and Astrophysics, Catalogues, Galaxy, Redshift, Data set, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), data analysi [methods], Magnitude (astronomy), Dark energy, catalogue, Galaxy morphological classification
Abstract

Cheng, Ting-Yun, et al., We present in this paper one of the largest galaxy morphological classification catalogues to date, including over 20 million galaxies, using the Dark Energy Survey (DES) Year 3 data based on convolutional neural networks (CNNs). Monochromatic i-band DES images with linear, logarithmic, and gradient scales, matched with debiased visual classifications from the Galaxy Zoo 1 (GZ1) catalogue, are used to train our CNN models. With a training set including bright galaxies (16 ≤ i < 18) at low redshift (z < 0.25), we furthermore investigate the limit of the accuracy of our predictions applied to galaxies at fainter magnitude and at higher redshifts. Our final catalogue covers magnitudes 16 ≤ i < 21, and redshifts z < 1.0, and provides predicted probabilities to two galaxy types – ellipticals and spirals (disc galaxies). Our CNN classifications reveal an accuracy of over 99 per cent for bright galaxies when comparing with the GZ1 classifications (i < 18). For fainter galaxies, the visual classification carried out by three of the co-authors shows that the CNN classifier correctly categorizes discy galaxies with rounder and blurred features, which humans often incorrectly visually classify as ellipticals. As a part of the validation, we carry out one of the largest examinations of non-parametric methods, including ∼100 ,000 galaxies with the same coverage of magnitude and redshift as the training set from our catalogue. We find that the Gini coefficient is the best single parameter discriminator between ellipticals and spirals for this data set., 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 MINECO under grants AYA2015- 71825, ESP2015-66861, FPA2015-68048, SEV-2016-0588, SEV2016-0597, 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 Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020, and the Brazilian Instituto Nacional de Ciencia e Tecnologia (INCT) e-Universe (CNPq grant 465376/2014-2).

Published
2021

404. A machine learning approach to galaxy properties: Joint redshift-stellar mass probability distributions with Random Forest

Author

A. A. Plazas, L. N. Da Costa, W. G. Hartley, Maria E. S. Pereira, Brian Yanny, Marcos Lima, Alex Drlica-Wagner, J. Carretero, Antonella Palmese, E. M. Huff, Juan Garcia-Bellido, Ramon Miquel, M. A. G. Maia, Michel Aguena, V. Scarpine, A. Choi, Martin Crocce, F. J. Castander, G. Tarle, R. D. Wilkinson, Ian Harrison, S. Mucesh, K. Honscheid, Sunayana Bhargava, A. Alarcon, J. De Vicente, David J. James, Huan Lin, Pablo Fosalba, M. Carrasco Kind, Chun-Hao To, Alexandra Amon, E. J. Sanchez, F. Paz-Chinchón, Keith Bechtol, E. Suchyta, August E. Evrard, M. Costanzi, M. Smith, Felipe Menanteau, Josh Frieman, D. L. Hollowood, S. Allam, Robert A. Gruendl, S. Serrano, Ofer Lahav, Daniel Gruen, Samuel Hinton, Peter Melchior, Christopher J. Conselice, Erin Sheldon, B. Flaugher, E. Bertin, G. Gutierrez, David J. Brooks, S. Desai, Enrique Gaztanaga, Robert Morgan, J. Gschwend, S. Everett, D. W. Gerdes, Gary Bernstein, I. Ferrero, H. T. Diehl, David Bacon, I. Sevilla-Noarbe, N. Kuropatkin, K. D. Eckert, T. N. Varga, Asa F. L. Bluck, Kyler Kuehn, Michael Schubnell, Daniel Thomas, L. Whiteway, A. Carnero Rosell, National Science Foundation (US), Ministerio de Ciencia, Innovación y Universidades (España), Generalitat de Catalunya, European Commission, Instituto Nacional de Ciência e Tecnologia (Brasil), 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, Mucesh, S., Hartley, W. G., Palmese, A., Lahav, O., Whiteway, L., Amon, A., Bechtol, K., Bernstein, G. M., Carnero Rosell, A., Carrasco Kind, M., Choi, A., Eckert, K., Everett, S., Gruen, D., Gruendl, R. A., Harrison, I., Huff, E. M., Kuropatkin, N., Sevilla-Noarbe, I., Sheldon, E., Yanny, B., Aguena, M., Allam, S., Bacon, D., Bertin, E., Bhargava, S., Brooks, D., Carretero, J., Castander, F. J., Conselice, C., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Diehl, H. T., Drlica-Wagner, A., Evrard, A. E., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., James, D. J., Kuehn, K., Lima, M., Lin, H., Maia, M. A. G., Melchior, P., Menanteau, F., Miquel, R., Morgan, R., Paz-Chinchón, F., Plazas, A. A., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Smith, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Varga, T. N., and Wilkinson, R. D.

Subjects
FOS: Computer and information sciences, Computer Science - Machine Learning, statistical [Methods], software: data analysis, computer.software_genre, 01 natural sciences, data analysi [software], Copula (probability theory), Machine Learning (cs.LG), Astrophysics - Cosmology and Nongalactic Astrophysic, data analysis [Methods], 010303 astronomy & astrophysics, Physics, fundamental parameter [galaxies], galaxies: fundamental parameters, Random forest, Software: public realese, fundamental parameters [Galaxies], Probability distribution, galaxies: evolution, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, public realese [Software], Cosmology and Nongalactic Astrophysics (astro-ph.CO), methods: data analysis, methods: statistical, software: public release, Astrophysics - Astrophysics of Galaxies, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Machine learning, Astrophysics - Astrophysics of Galaxie, 0103 physical sciences, Galaxy formation and evolution, [INFO]Computer Science [cs], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Probability integral transform, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010308 nuclear & particles physics, business.industry, Univariate, Astronomy and Astrophysics, evolution [Galaxies], public release [software], Redshift, Galaxy, Space and Planetary Science, data analysis [Software], Astrophysics of Galaxies (astro-ph.GA), data analysi [methods], Artificial intelligence, Astrophysics - Instrumentation and Methods for Astrophysic, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], business, computer
Abstract

We demonstrate that highly accurate joint redshift-stellar mass probability distribution functions (PDFs) can be obtained using the Random Forest (RF) machine learning (ML) algorithm, even with few photometric bands available. As an example, we use the Dark Energy Survey (DES), combined with the COSMOS2015 catalogue for redshifts and stellar masses. We build two ML models: one containing deep photometry in the $griz$ bands, and the second reflecting the photometric scatter present in the main DES survey, with carefully constructed representative training data in each case. We validate our joint PDFs for $10,699$ test galaxies by utilizing the copula probability integral transform and the Kendall distribution function, and their univariate counterparts to validate the marginals. Benchmarked against a basic set-up of the template-fitting code BAGPIPES, our ML-based method outperforms template fitting on all of our predefined performance metrics. In addition to accuracy, the RF is extremely fast, able to compute joint PDFs for a million galaxies in just under $6$ min with consumer computer hardware. Such speed enables PDFs to be derived in real time within analysis codes, solving potential storage issues. As part of this work we have developed GALPRO, a highly intuitive and efficient Python package to rapidly generate multivariate PDFs on-the-fly. GALPRO is documented and available for researchers to use in their cosmology and galaxy evolution studies., Comment: 18 pages, 8 figures, Accepted by MNRAS

Published
2021
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405. Dark energy survey year 1 results: The lensing imprint of cosmic voids on the cosmic microwave background

Author

Marcos Lima, David J. Brooks, Ofer Lahav, D. L. Hollowood, S. Serrano, J. De Vicente, Dragan Huterer, J. Carretero, Seshadri Nadathur, A. A. Plazas, Peter Melchior, Felipe Menanteau, J. Annis, Daniel Thomas, Joe Zuntz, L. Whiteway, J. Gschwend, M. Costanzi, M. March, P. Vielzeuf, Eric J. Baxter, M. Smith, Josh Frieman, E. Suchyta, Jennifer L. Marshall, Carlos Solans Sanchez, A. Carnero Rosell, Tim Eifler, Daniel Gruen, Nico Hamaus, G. Tarle, A. Kovács, B. Flaugher, S. Everett, D. W. Gerdes, K. Honscheid, W. G. Hartley, Santiago Avila, Antonella Palmese, Ramon Miquel, F. Paz-Chinchón, M. A. G. Maia, Jochen Weller, Juan Garcia-Bellido, V. Scarpine, U. Demirbozan, Peter Doel, T. M. C. Abbott, H. T. Diehl, E. J. Sanchez, G. Gutierrez, David J. James, Pablo Fosalba, G. Pollina, Shantanu Desai, I. Sevilla-Noarbe, N. Kuropatkin, L. N. da Costa, Enrique Gaztanaga, R. Cawthon, M. Carrasco Kind, Kyler Kuehn, D. L. Burke, S. Allam, Robert A. Gruendl, Ministerio de Ciencia e Innovación (España), European Commission, UAM. Departamento de Física Teórica, Vielzeuf, P, Kovács, A, Demirbozan, U, Fosalba, P, Baxter, E, Hamaus, N, Huterer, D, Miquel, R, Nadathur, S, Pollina, G, Sánchez, C, Whiteway, L, Abbott, T M C, Allam, S, Annis, J, Avila, S, Brooks, D, Burke, D L, Rosell, A Carnero, Kind, M Carrasco, Carretero, J, Cawthon, R, Costanzi, M, da Costa, L N, De Vicente, J, Desai, S, Diehl, H T, Doel, P, Eifler, T F, Everett, S, Flaugher, B, Frieman, J, García-Bellido, J, Gaztanaga, E, Gerdes, D W, Gruen, D, Gruendl, R A, Gschwend, J, Gutierrez, G, Hartley, W G, Hollowood, D L, Honscheid, K, James, D J, Kuehn, K, Kuropatkin, N, Lahav, O, Lima, M, Maia, M A G, March, M, Marshall, J L, Melchior, P, Menanteau, F, Palmese, A, Paz-Chinchón, F, Plazas, A A, Sanchez, E, Scarpine, V, Serrano, S, Sevilla-Noarbe, I, Smith, M, Suchyta, E, Tarle, G, Thomas, D, Weller, J, and Zuntz, J

Subjects
Void (astronomy), Cosmology and Nongalactic Astrophysics (astro-ph.CO), Large-scale structure of Universe, Cosmic microwave background, Cosmic background radiation, FOS: Physical sciences, Astrophysics, cosmic background radiation, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, 7. Clean energy, symbols.namesake, TRACER, 0103 physical sciences, LENTES GRAVITACIONAIS, Planck, 010303 astronomy & astrophysics, STFC, Physics, COSMIC cancer database, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, Física, RCUK, Astronomy and Astrophysics, Galaxy, 13. Climate action, Space and Planetary Science, Dark energy, symbols, large-scale structure of Universe, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Cosmic voids gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint on degree scales. We use the simulated CMB lensing convergence map from the Marenostrum Institut de Ciencias de l’Espai (MICE) N-body simulation to calibrate our detection strategy for a given void definition and galaxy tracer density. We then identify cosmic voids in Dark Energy Survey (DES) Year 1 data and stack the Planck 2015 lensing convergence map on their locations, probing the consistency of simulated and observed void lensing signals. When fixing the shape of the stacked convergence profile to that calibrated from simulations, we find imprints at the 3σ significance level for various analysis choices. The best measurement strategies based on the MICE calibration process yield S/N ≈ 4 for DES Y1, and the best-fitting amplitude recovered from the data is consistent with expectations from MICE (A ≈ 1). Given these results as well as the agreement between them and N-body simulations, we conclude that the previously reported excess integrated Sachs–Wolfe (ISW) signal associated with cosmic voids in DES Y1 has no counterpart in the Planck CMB lensing map., This work has made use of CosmoHub (see Carretero et al. 2017). CosmoHub has been developed by the Port d’Informacio Cient ´ ´ıfica (PIC), maintained through a collaboration of the Institut de F´ısica d’Altes Energies (IFAE) and the Centro de Investigaciones Energeticas, Medioambientales y Tecnol ´ ogicas (CIEMAT), and was ´ partially funded by the ‘Plan Estatal de Investigacion Cient ´ ´ıfica y Tecnica y de Innovaci ´ on’ program of the Spanish government. ´ Funding for the DES Projects has been provided by the US Department of Energy, the US 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, Fundac¸ao Carlos Chagas Filho de Amparo ˜ a Pesquisa do ` Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Cient´ıfico e Tecnologico and the Minist ´ erio da Ci ´ encia, Tecnologia ˆ e Inovac¸ao, the Deutsche Forschungsgemeinschaft, and the Collab- ˜ orating 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, Medioambien- ´ tales y Tecnologicas-Madrid, the University of Chicago, Univer- ´ sity College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenossische 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 F´ısica d’Altes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universitat¨ Munchen and the associated Excellence Cluster Universe, the Uni- ¨ versity 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. This paper is based in part on observations at Cerro Tololo InterAmerican 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 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 MINECO under grants AYA2015- 71825, ESP2015-66861, FPA2015-68048, SEV-2016-0588, SEV2016-0597, 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, 306478, and 615929. We acknowledge support from the Brazilian Instituto Nacional de Cienciae Tecnologia ˆ (INCT) e-Universe (CNPq grant 465376/2014-2). This paper has been authored by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the US Department of Energy, Office of Science, Office of High Energy Physics. PV acknowledges the support from the grant MIUR PRIN 2015 ‘Cosmology and Fundamental Physics: illuminating the Dark Universe with Euclid’. AK has been supported by a Juan de la Cierva fellowship from MINECO with project number IJC2018-037730-I. Funding for this project was also available in part through SEV-2015-0548 and AYA2017-89891-P. This project has also received funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 754558.

Published
2021
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406. Dark energy survey internal consistency tests of the joint cosmological probes analysis with posterior predictive distributions

Author

R. L. C. Ogando, J. DeRose, E. Suchyta, M. Smith, G. Tarle, Daniel Gruen, Youngsoo Park, D. W. Gerdes, S. Samuroff, T. N. Varga, R. Cawthon, David J. Brooks, J. Gschwend, Sunayana Bhargava, Michael Schubnell, K. Honscheid, Samuel Hinton, W. G. Hartley, Marcos Lima, J. P. Dietrich, G. Gutierrez, Ofer Lahav, Juan Garcia-Bellido, C. Lidman, Alexandra Amon, J. Carretero, Ramon Miquel, Peter Doel, M. Costanzi, Dragan Huterer, M. Carrasco Kind, Robert Morgan, J. Frieman, H. T. Diehl, David Bacon, Felipe Menanteau, E. Baxter, F. Paz-Chinchón, I. Ferrero, Matt J. Jarvis, J. Annis, Marco Raveri, Elisabeth Krause, M. Gatti, David J. James, Niall MacCrann, J. Muir, Tommaso Giannantonio, D. L. Burke, Pablo Fosalba, Ami Choi, Ben Hoyle, E. Bertin, A. A. Plazas, I. Sevilla-Noarbe, Bhuvnesh Jain, S. Allam, Robert A. Gruendl, V. Scarpine, Antonella Palmese, N. Kuropatkin, D. L. Hollowood, M. A. G. Maia, S. Serrano, A. Alarcon, A. Campos, E. M. Huff, L. N. da Costa, P. Lemos, Michel Aguena, R. D. Wilkinson, S. Everett, Maria E. S. Pereira, J. Prat, M. E. C. Swanson, Jochen Weller, T. M. C. Abbott, C. Doux, Chun-Hao To, Markus Rau, E. J. Sanchez, Santiago Avila, Chihway Chang, Michael Troxel, S. Desai, Joe Zuntz, Douglas L. Tucker, Kyler Kuehn, National Science Foundation (US), Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), European Commission, Generalitat de Catalunya, Instituto Nacional de Ciência e Tecnologia (Brasil), Fermilab, Doux, C., Baxter, E., Lemos, P., Chang, C., Alarcon, A., Amon, A., Campos, A., Choi, A., Gatti, M., Gruen, D., Jarvis, M., Maccrann, N., Park, Y., Prat, J., Rau, M. M., Raveri, M., Samuroff, S., Derose, J., Hartley, W. G., Hoyle, B., Troxel, M. A., Zuntz, J., Abbott, T. M. C., Aguena, M., Allam, S., Annis, J., Avila, S., Bacon, D., Bertin, E., Bhargava, S., Brooks, D., Burke, D. L., Carrasco Kind, M., Carretero, J., Cawthon, R., Costanzi, M., da Costa, L. N., Pereira, M. E. S., Desai, S., Diehl, H. T., Dietrich, J. P., Doel, P., Everett, S., Ferrero, I., Fosalba, P., 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., Huff, E. M., Huterer, D., Jain, B., James, D. J., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lidman, C., Lima, M., Maia, M. A. G., Menanteau, F., Miquel, R., Morgan, R., Muir, J., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., To, C., Tucker, D. L., Varga, T. N., Weller, J., 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
statistical [Methods], Cosmology and Nongalactic Astrophysics (astro-ph.CO), Large-scale structure of Universe, FOS: Physical sciences, Dark energy, Gravitational lensing: weak, Methods: statistical, gravitational lensing: weak, methods: statistical, dark energy, large-scale structure of Universe, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, 01 natural sciences, Data vector, Goodness of fit, Consistency (statistics), Internal consistency, 0103 physical sciences, Statistics, Astrophysics - Cosmology and Nongalactic Astrophysic, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010303 astronomy & astrophysics, Joint (geology), Instrumentation and Methods for Astrophysics (astro-ph.IM), Physics, 010308 nuclear & particles physics, Astronomy and Astrophysics, Data set, Posterior predictive distribution, Space and Planetary Science, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], weak [Gravitational lensing]
Abstract

Doux, C., et al. DES Collaboration, Beyond ΛCDM, physics or systematic errors may cause subsets of a cosmological data set to appear inconsistent when analysed assuming ΛCDM. We present an application of internal consistency tests to measurements from the Dark Energy Survey Year 1 (DES Y1) joint probes analysis. Our analysis relies on computing the posterior predictive distribution (PPD) for these data under the assumption of ΛCDM. We find that the DES Y1 data have an acceptable goodness of fit to ΛCDM, with a probability of finding a worse fit by random chance of p = 0.046. Using numerical PPD tests, supplemented by graphical checks, we show that most of the data vector appears completely consistent with expectations, although we observe a small tension between large- and small-scale measurements. A small part (roughly 1.5 per cent) of the data vector shows an unusually large departure from expectations; excluding this part of the data has negligible impact on cosmological constraints, but does significantly improve the p-value to 0.10. The methodology developed here will be applied to test the consistency of DES Year 3 joint probes data sets., 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
2021
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407. OzDES Reverberation Mapping Programme: The first Mg ii lags from 5 yr of monitoring

Author

I. Ferrero, Antonella Palmese, I. Sevilla-Noarbe, M. Soares-Santos, Paul Martini, N. Kuropatkin, Zhefu Yu, M. A. G. Maia, J. Calcino, B. Flaugher, Josh Frieman, David J. James, A. Penton, L. N. da Costa, Anais Möller, M. March, A. G. Kim, Bradley M. Peterson, Ramon Miquel, A. A. Plazas, E. Bertin, Tamara M. Davis, Geraint F. Lewis, Juan Garcia-Bellido, Douglas L. Tucker, Kyler Kuehn, Rob Sharp, H. T. Diehl, Jacobo Asorey, C. Lidman, B. E. Tucker, J. Annis, D. L. Burke, D. L. Hollowood, S. Serrano, M.E. da Silva Pereira, M. Smith, M. Costanzi, Robert Morgan, Daniel Gruen, Enrique Gaztanaga, S. Allam, Robert A. Gruendl, D. W. Gerdes, G. Tarle, Jennifer L. Marshall, J. Gschwend, V. Scarpine, Daniel Thomas, S. Everett, Michel Aguena, Christopher S. Kochanek, Daniela Carollo, F. Paz-Chinchón, U. Malik, M. Carrasco Kind, F. Andrade-Oliveira, Samuel Hinton, G. Gutierrez, Richard G. Kron, Felipe Menanteau, E. Suchyta, David J. Brooks, A. Carnero Rosell, Chun-Hao To, E. J. Sanchez, Yu, Z., Martini, P., Penton, A., Davis, T. M., Malik, U., Lidman, C., Tucker, B. E., Sharp, R., Kochanek, C. S., Peterson, B. M., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Asorey, J., Bertin, E., Brooks, D., Burke, D. L., Calcino, J., Carnero Rosell, A., Carollo, D., Carrasco Kind, M., Costanzi, M., Da Costa, L. N., Da Silva Pereira, M. E. S., Diehl, H. T., Everett, S., Ferrero, I., Flaugher, B., Frieman, J., Garcia-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., James, D. J., Kim, A. G., Kron, R., Kuehn, K., Kuropatkin, N., Lewis, G. F., Maia, M. A. G., March, M., Marshall, J. L., Menanteau, F., Miquel, R., Morgan, R., Moller, A., Palmese, A., Paz-Chinchon, F., Plazas, A. A., Sanchez, E., Scarpine, V., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Tucker, D. L., The Ohio State University, Harvard University, University of Queensland, ARC Centre of Excellence for All-sky Astrophysics (CAASTRO), Australian National University, Australian Astronomical Observatory, 3700 San Martin Drive, Universidade de São Paulo (USP), LineA, Fermi National Accelerator Laboratory, Universidade Estadual Paulista (UNESP), Medioambientales y Tecnológicas (CIEMAT), Institut D'Astrophysique DeParis, Institutd'Astrophysique de Paris, Gower Street, SLAC National Accelerator Laboratory, Stanford University, Instituto de Astrofisica de Canarias, Dpto. Astrofísica, Astrophysical Observatory of Turin, National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign, University of Trieste, Osservatorio Astronomico di Trieste, Institute for Fundamental Physics of the Universe, Observatório Nacional, University of Michigan, Santa Cruz Institute for Particle Physics, University of Oslo, University of Chicago, Universidad Autonoma de Madrid, CSIC), Institut D'Estudis Espacials de Catalunya (IEEC), Harvard & Smithsonian, Lawrence Berkeley National Laboratory, Lowell Observatory, the University of Sydney, University of Pennsylvania, Texas A&M University, Institució Catalana de Recerca i Estudis Avancats, The Barcelona Institute of Science and Technology Campus UAB, University of Wisconsin- Madison, LPC, University of Cambridge, Peyton Hall, University of Southampton, Oak Ridge National Laboratory, University of Portsmouth, National Science Foundation (US), Department of Energy (US), Australian Government, Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), Generalitat de Catalunya, European Commission, Instituto Nacional de Ciência e Tecnologia (Brasil), 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), 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), and OzDES

Subjects
Physics, Supermassive black hole, general [quasars], 010308 nuclear & particles physics, Lag, nuclei [galaxies], Astronomy and Astrophysics, Quasar, Astrophysics, galaxies: nuclei, quasars: general, 01 natural sciences, Spectral line, Space and Planetary Science, 0103 physical sciences, Reverberation mapping, Emission spectrum, Continuum (set theory), [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 010303 astronomy & astrophysics, Line (formation)
Abstract

Yu, Zhefu, et al., Reverberation mapping is a robust method to measure the masses of supermassive black holes outside of the local Universe. Measurements of the radius–luminosity (R−L) relation using the Mg II emission line are critical for determining these masses near the peak of quasar activity at z ≈ 1−2, and for calibrating secondary mass estimators based on Mg II that can be applied to large samples with only single-epoch spectroscopy. We present the first nine Mg II lags from our 5-yr Australian Dark Energy Survey reverberation mapping programme, which substantially improves the number and quality of Mg II lag measurements. As the Mg II feature is somewhat blended with iron emission, we model and subtract both the continuum and iron contamination from the multiepoch spectra before analysing the Mg II line. We also develop a new method of quantifying correlated spectroscopic calibration errors based on our numerous, contemporaneous observations of F-stars. The lag measurements for seven of our nine sources are consistent with both the H β and Mg II R−L relations reported by previous studies. Our simulations verify the lag reliability of our nine measurements, and we estimate that the median false positive rate of the lag measurements is 4 per cent⁠., We thank the anonymous referee for the careful review and comments. We thank Dr. Yue Shen for the constructive comments. ZY was supported in part by the United States National Science Foundation under Grant No. 161553 to PM. PM is grateful for support from the Radcliffe Institute for Advanced Study at Harvard University. PM also acknowledges support from the United States Department of Energy, Office of High Energy Physics under Award Number DE-SC-0011726. AP and UM are supported by the Australian Government Research Training Programme (RTP) Scholarship. This research was supported in part by the Australian Government through the Australian Research Council Laureate Fellowship funding scheme (project FL180100168). Based in part on data acquired at the Anglo-Australian Telescope, under programme A/2013B/012]. We acknowledge the traditional owners of the land on which the AAT stands, the Gamilaroi people, and pay our respects to elders past and present. 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 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 Programme (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
2021
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409. Dark Energy Survey Year 3 results: Curved-sky weak lensing mass map reconstruction

Author

Sunayana Bhargava, Jennifer L. Marshall, David J. Brooks, Carlos Solans Sanchez, G. Tarle, Samuel Hinton, G. Gutierrez, Alexandra Amon, Peter Doel, Ami Choi, Ben Hoyle, Marco Raveri, B. Flaugher, F. Andrade-Oliveira, Jochen Weller, R. P. Rollins, H. T. Diehl, D. L. Burke, Felipe Menanteau, Alex Drlica-Wagner, J. DeRose, F. J. Castander, David Bacon, E. Suchyta, Dragan Huterer, Christopher J. Conselice, Brian Yanny, Jack Elvin-Poole, U. Demirbozan, Maria E. S. Pereira, Niall MacCrann, Keith Bechtol, Erin Sheldon, Martin Crocce, V. Scarpine, T. M. C. Abbott, Peter Melchior, D. L. Hollowood, S. Serrano, Agnès Ferté, J. De Vicente, J. Cordero, P. F. Leget, A. Campos, Eli S. Rykoff, C. Doux, Chun-Hao To, E. J. Sanchez, K. Herner, F. Paz-Chinchón, J. Carretero, Antonella Palmese, Marcos Lima, J. Myles, I. Harrison, G. Pollina, A. Roodman, David J. James, Tommaso Giannantonio, D. Zeurcher, M. A. G. Maia, M. Rodriguez-Monroy, Joe Zuntz, A. Alarcon, B. Yin, S. Allam, Robert A. Gruendl, A. Kovács, Matthew R. Becker, Pablo Fosalba, B. Mawdsley, Ashley J. Ross, S. Pandey, J. Muir, Joseph J. Mohr, Michael Troxel, I. Ferrero, Matt J. Jarvis, A. Carnero Rosell, J. McCullough, P. Vielzeuf, Yanxi Zhang, Seshadri Nadathur, M. Carrasco Kind, M. March, S. Everett, M. Smith, M. Costanzi, Jean-Luc Starck, Daniel Gruen, I. Tutusaus, Francois Lanusse, Chihway Chang, Daniel Thomas, J. Prat, L. Whiteway, F. Elsner, S. Desai, I. Sevilla-Noarbe, M. Soares-Santos, G. Giannini, W. G. Hartley, D. W. Gerdes, R. Cawthon, N. Kuropatkin, Ramon Miquel, K. D. Eckert, T. N. Varga, L. N. da Costa, J. P. Dietrich, Juan Garcia-Bellido, E. Bertin, E. M. Huff, R. Chen, Michel Aguena, Enrique Gaztanaga, R. L. C. Ogando, Bhuvnesh Jain, M Gatti, Ofer Lahav, Niall Jeffrey, Robert Morgan, L. F. Secco, Nico Hamaus, A. A. Plazas, A. Navarro-Alsina, T. Shin, T. Kacprzak, C. Davis, J. Gschwend, Gary Bernstein, National Science Foundation (US), Ministerio de Ciencia, Innovación y Universidades (España), Ministerio de Economía y Competitividad (España), Generalitat de Catalunya, European Commission, Instituto Nacional de Ciência e Tecnologia (Brasil), University of Portsmouth, 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), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-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, 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), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Jeffrey, N., Gatti, M., Chang, C., Whiteway, L., Demirbozan, U., Kovacs, A., Pollina, G., Bacon, D., Hamaus, N., Kacprzak, T., Lahav, O., Lanusse, F., Mawdsley, B., Nadathur, S., Starck, J. L., Vielzeuf, P., Zeurcher, D., Alarcon, A., Amon, A., Bechtol, K., Bernstein, G. M., Campos, A., Rosell, A. C., Kind, M. C., 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., Ferte, 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., Sanchez, 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., Abbott, T. M. C., Aguena, M., Allam, S., Andrade-Oliveira, F., Becker, M. R., Bertin, E., Bhargava, S., Brooks, D., Burke, D. L., Carretero, J., Castander, F. J., Conselice, C., 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., Ferrero, I., Flaugher, B., Fosalba, P., Garcia-Bellido, J., Gaztanaga, E., Gerdes, D. W., Giannantonio, T., Gschwend, J., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Hoyle, B., Jain, B., James, D. J., Lima, M., Maia, M. A. G., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Ogando, R. L. C., Palmese, A., Paz-Chinchon, F., Plazas, A. A., Rodriguez-Monroy, M., Roodman, A., Sanchez, E., Scarpine, V., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Thomas, D., To, C., Weller, J., Université de Paris, University College London, Barcelona Institute of Science and Technology, University of Pennsylvania, University of Chicago, Calle Viá Láctea, Universidad de La Laguna (ULL), Ludwig-Maximilians Universität München, ETH Zurich, Argonne National Laboratory, Stanford University, University of Wisconsin-Madison, CarnegieMellon University, Instituto de Astrofisica de Canarias, Laboratorio Interinstitucional de e-Astronomia-LIneA, Dpto. Astrofisica, National Center for Supercomputing Applications, University of Illinois at Urbana-Champaign, Duke University, Ohio State University, University of Manchester, University of California,Berkeley, Santa Cruz Institute for Particle Physics, Fermi National Accelerator Laboratory, California Institute of Technology, SLAC National Accelerator Laboratory, Denys Wilkinson Building, University of Geneva, University of Michigan, University of Cambridge, Universidade Estadual de Campinas (UNICAMP), Medioambientales y Tecnologicas (CIEMAT), Brookhaven National Laboratory, Institut d'Estudis Espacials de Catalunya (IEEC), CSIC), Max Planck Institute for Extraterrestrial Physics, University of Edinburgh, NSF's National Optical-Infrared Astronomy Research Laboratory, Universidade de Saõ Paul, Universidade Estadual Paulista (UNESP), Institut d'Astrophysique deParis, Institut d'Astrophysique de Paris, University of Sussex, School of Physics and Astronomy, University of Trieste, INAF-Osservatorio Astronomico di Trieste, Institute for Fundamental Physics of the Universe, Observatório Nacional, IIT Hyderabad, Ludwig-Maximilians-Universitat, University of Oslo, Universidad Autonoma de Madrid, University of Queensland, Center for Astrophysics | Harvard and Smithsonian, Texas A and M University, Princeton University, Institucio Catalana de Recerca i Estudis Avancats, University of Southampton, Oak Ridge National Laboratory, and Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Sorbonne Université (SU)-École normale supérieure - Paris (ENS Paris)

Subjects
statistical [Methods], Cosmology and Nongalactic Astrophysics (astro-ph.CO), media_common.quotation_subject, Dark matter, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 7. Clean energy, 01 natural sciences, Gravitational lensing: weak, 0103 physical sciences, Prior probability, Maximum a posteriori estimation, 010303 astronomy & astrophysics, STFC, Weak gravitational lensing, Methods: statistical, media_common, Physics, ST/M001334/1, 010308 nuclear & particles physics, RCUK, Astronomy and Astrophysics, Celestial sphere, gravitational lensing: Weak, large-scale structure of Universe, methods: Statistical, ST/R000476/1, Galaxy, Space and Planetary Science, Sky, astro-ph.CO, Dark energy, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], weak [Gravitational lensing], Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Jeffrey, N., et al. DES Collaboration, We present reconstructed convergence maps, mass maps, from the Dark Energy Survey (DES) third year (Y3) weak gravitational lensing data set. The mass maps are weighted projections of the density field (primarily dark matter) in the foreground of the observed galaxies. We use four reconstruction methods, each is a maximum a posteriori estimate with a different model for the prior probability of the map: Kaiser–Squires, null B-mode prior, Gaussian prior, and a sparsity prior. All methods are implemented on the celestial sphere to accommodate the large sky coverage of the DES Y3 data. We compare the methods using realistic ΛCDM simulations with mock data that are closely matched to the DES Y3 data. We quantify the performance of the methods at the map level and then apply the reconstruction methods to the DES Y3 data, performing tests for systematic error effects. The maps are compared with optical foreground cosmic-web structures and are used to evaluate the lensing signal from cosmic-void profiles. The recovered dark matter map covers the largest sky fraction of any galaxy weak lensing map to date., 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 paper 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. NJ has been supported by funding from l’Ecole Normale Supérieure, Paris. OL and NJ acknowledge support from a European Research Council Advanced Grant TESTDE (FP7/291329) and STFC Consolidated Grants ST/M001334/1 and ST/R000476/1. AK has been supported by a Juan de la Cierva fellowship from MINECO with project number IJC2018-037730-I, and funding for this project was also available in part through SEV-2015-0548 and AYA2017-89891-P. Cosmic voids computational work has been performed on the UK SCIAMA High Performance Computing cluster supported by the ICG, SEPNet, and the University of Portsmouth.

Published
2021
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410. Phenological analysis through the use of multitemporal TLS observation

Author

Pascu, Ionut Silviu, Alexandru-Claudiu Dobre, Zamfira, Virgil, Apostol, Ecaterina, Leca, Stefan, Pitar, Diana, Apostol, Bogdan, Chivulescu, Serban, Ciceu, Albert, Duro, Juan Garcia, and Badea, Ovidiu

Abstract

The current paper tested the hypothesis that TLS through its high accuracy, increased spatial resolution, portability, equivalenting în high temporal resolution, automated processing and unlimited revisiting capabilities of the scene once record ed, might represent the best available technology for phenological evaluation. Phenology observations represent one of the most accurate methods for evaluating the response of plant species to various climate conditions and climate changes. The main objective of this research was to identify the pattems pf early vegetation stages in the context of a reduced precipitation regime through terrestrial scanning technique. The research was carried out in a mixed forest stand ( Carpinus betulus, Acer campestre, Tilia cordata, Quercus robur) with the focus of more precisely identifying the pattem of early vegetation development. The phenological processes analysis was done at an increased spatial and temporal resolution, on specific horizontal layers by means of terrestrial laser scanning. With a daily cycle started in March, we maintained a constant scanning position as well as time of day and scanning resolution. Supervised thresholds have been set at the heights of separation between undergrowth, trunk and crown, and for each resulting layer coverage and density metrics as well as derived indices (Gap Fraction and Leaf Area Density) have been computed. For reference data, photos were interpreted as per the ICP Forests guideline. A sequential evolution was observed în all studied species. Hornbeam displayed a daily increase în LAD for all layers up until epicormic branches shadowing overtook the upper canopy visibility. Small-leaved lime showed a delay of almost 20 days in comparison to oak. Oak started with an abrupt 13% increase in foliage volume from the reference date, compared to the 3% increase în the small-leaved lime. Also, at the time of bud flushing of the small-leaved lime, the oak had already been through four similar stages (18-20-23%). Although not identica! to the historical data, analysed trends still fit the expected pattems.

Published
2021
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411. Pushing automated morphological classifications to their limits with the Dark Energy Survey

Author

Mariangela Bernardi, E. Suchyta, J. Carretero, M. Carrasco Kind, Christopher J. Conselice, A. G. Kim, A. Carnero Rosell, Felipe Menanteau, Marc Huertas-Company, E. Bertin, W. G. Hartley, I. Ferrero, Matt J. Jarvis, David J. Brooks, Jesús Vega-Ferrero, Samuel Hinton, Josh Frieman, J. Gschwend, M. E. C. Swanson, M. Smith, G. Gutierrez, D. L. Hollowood, Pablo Fosalba, R. L. C. Ogando, S. Serrano, Santiago Avila, Daniel Gruen, Ramon Miquel, H. Domínguez Sánchez, V. Scarpine, A. Choi, I. Sevilla-Noarbe, K. Honscheid, N. Kuropatkin, T. N. Varga, S. Desai, David Bacon, L. N. da Costa, S. Allam, Marcos Lima, G. Tarle, Michael Schubnell, Robert A. Gruendl, Ben Hoyle, Maria E. S. Pereira, Chun-Hao To, E. J. Sanchez, Antonella Palmese, B. Margalef, M. A. G. Maia, Michel Aguena, Robert Morgan, F. Tarsitano, F. Paz-Chinchón, A. K. Romer, J. De Vicente, A. A. Plazas, Douglas L. Tucker, Kyler Kuehn, M. Costanzi, R. D. Wilkinson, Juan Garcia-Bellido, J. Annis, National Science Foundation (US), Ministerio de Ciencia, Innovación y Universidades (España), Ministerio de Economía y Competitividad (España), European Commission, Generalitat de Catalunya, Instituto Nacional de Ciência e Tecnologia (Brasil), Vega-Ferrero, J., Domínguez Sánchez, H., Bernardi, M., Huertas-Company, M., Morgan, R., Margalef, B., Aguena, M., Allam, S., Annis, J., Avila, S., Bacon, D., Bertin, E., Brooks, D., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Choi, A., Conselice, C., Costanzi, M., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Ferrero, I., Fosalba, P., Frieman, J., García-Bellido, J., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., Jarvis, M., Kim, A. G., Kuehn, K., Kuropatkin, N., Lima, M., Maia, M. A. G., Menanteau, F., Miquel, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Romer, A. K., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Tarsitano, F., To, C., Tucker, D. L., Varga, T. N., Wilkinson, R. D., Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA (UMR_8112)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-CY Cergy Paris Université (CY), 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, Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-CY Cergy Paris Université (CY)

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), structure [Galaxies], FOS: Physical sciences, Classification scheme, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Convolutional neural network, Astrophysics - Astrophysics of Galaxie, 0103 physical sciences, observational [Methods], 010303 astronomy & astrophysics, Lenticular galaxy, catalogues, Astrophysics::Galaxy Astrophysics, Physics, 010308 nuclear & particles physics, business.industry, Deep learning, Astronomy and Astrophysics, Pattern recognition, Catalogues, Astrophysics - Astrophysics of Galaxies, Galaxy, Redshift, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Dark energy, galaxies: structure, Artificial intelligence, methods: observational, Astrophysics - Cosmology and Nongalactic Astrophysics, catalogue, business, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Data release
Abstract

Vega-Ferrero, J., et al., We present morphological classifications of ∼27 million galaxies from the Dark Energy Survey (DES) Data Release 1 (DR1) using a supervised deep learning algorithm. The classification scheme separates: (a) early-type galaxies (ETGs) from late-type galaxies (LTGs); and (b) face-on galaxies from edge-on. Our convolutional neural networks (CNNs) are trained on a small subset of DES objects with previously known classifications. These typically have mr ≲ 17.7 mag; we model fainter objects to mr < 21.5 mag by simulating what the brighter objects with well-determined classifications would look like if they were at higher redshifts. The CNNs reach 97 per cent accuracy to mr < 21.5 on their training sets, suggesting that they are able to recover features more accurately than the human eye. We then used the trained CNNs to classify the vast majority of the other DES images. The final catalogue comprises five independent CNN predictions for each classification scheme, helping to determine if the CNN predictions are robust or not. We obtain secure classifications for ∼87 per cent and 73 per cent of the catalogue for the ETG versus LTG and edge-on versus face-on models, respectively. Combining the two classifications (a) and (b) helps to increase the purity of the ETG sample and to identify edge-on lenticular galaxies (as ETGs with high ellipticity). Where a comparison is possible, our classifications correlate very well with Sérsic index (n), ellipticity (ϵ), and spectral type, even for the fainter galaxies. This is the largest multiband catalogue of automated galaxy morphologies to date., 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
2021
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412. Cosmic conundra explained by thermal history and primordial black holes

Author

Bernard Carr, Juan Garcia-Bellido, Sebastien Clesse, Florian Kuhnel, and UAM. Departamento de Física Teórica

Subjects
High Energy Physics - Theory, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Black Holes, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, FOS: Physical sciences, Primordial black holes, Quark–hadron transition, Primordial black hole, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Compact star, 01 natural sciences, General Relativity and Quantum Cosmology, High Energy Physics - Phenomenology (hep-ph), Big Bang nucleosynthesis, 0103 physical sciences, Dark Matter, EW transition, 010303 astronomy & astrophysics, Astrophysique, Cosmologie, Astrophysics::Galaxy Astrophysics, Physics, Gravitational Waves, Supermassive black hole, 010308 nuclear & particles physics, Primordial nucleosynthesis, Física, Astronomy and Astrophysics, Astronomie, Informatique médicale, Redshift, LIGO, Black hole, High Energy Physics - Phenomenology, High Energy Physics - Theory (hep-th), Space and Planetary Science, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

A universal mechanism may be responsible for several unresolved cosmic conundra. The sudden drop in the pressure of relativistic matter at W±∕Z0 decoupling, the quark–hadron transition and e+e− annihilation enhances the probability of primordial black hole (PBH) formation in the early Universe. Assuming the amplitude of the primordial curvature fluctuations is approximately scale-invariant, this implies a multi-modal PBH mass spectrum with peaks at 10−6, 1, 30, and 106M⊙. This suggests a unified PBH scenario which naturally explains the dark matter and recent microlensing observations, the LIGO/Virgo black hole mergers, the correlations in the cosmic infrared and X-ray backgrounds, and the origin of the supermassive black holes in galactic nuclei at high redshift. A distinctive prediction of our model is that LIGO/Virgo should observe black hole mergers in the mass gaps between 2 and 5M⊙ (where no stellar remnants are expected) and above 65M⊙ (where pair-instability supernovae occur) and low-mass-ratios in between. Therefore the recent detection of events GW190425, GW190814 and GW190521 with these features is striking confirmation of our prediction and may indicate a primordial origin for the black holes. In this case, the exponential sensitivity of the PBH abundance to the equation of state would offer a unique probe of the QCD phase transition. The detection of PBHs would also offer a novel way to probe the existence of new particles or phase transitions with energy between 1MeV and 1010GeV., SCOPUS: ar.j, info:eu-repo/semantics/published

Published
2021

413. “Fatty Lungs”: An uncommon case of Autoimmune Pulmonary Alveolar Proteinosis

Author

Arnaldo A, Nieves-Ortiz, primary, Kyomara, Hernandez-Moya, additional, Juan, Garcia-Puebla, additional, Kimberly, Padilla-Rodriguez, additional, Neshma, Roman-Velez, additional, Giovanni, Veloz-Irizarry, additional, Keren, Mendez-Ramirez, additional, Hector, Collazo-Santiago, additional, Jose, Adorno-Fontanez, additional, and Ricardo, Fernandez-Gonzalez, additional

Published
2021
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415. Clinical effectiveness of olaparib monotherapy in germline BRCA-mutated, HER2-negative metastatic breast cancer in a real-world setting: phase IIIb LUCY interim analysis

Author

Karen A. Gelmon, Peter A. Fasching, Fergus J. Couch, Judith Balmaña, Suzette Delaloge, Intidhar Labidi-Galy, James Bennett, Susan McCutcheon, Graham Walker, Joyce O'Shaughnessy, Constanta Timcheva, Antoaneta Tomova, Andrea Eisen, Karen Gelmon, Julie Lemieux, Fernando Bazan, Hugues Bourgeois, Camille Chakiba, Mohamad Chehimi, Florence Dalenc, Thibault De La Motte Rouge, Jean-Sébastien Frenel, Anthony Gonçalves, Anne Claire Hardy-Bessard, Regine Lamy, Christelle Levy, Alain Lortholary, Audrey Mailliez, Jacques Medioni, Anne Patsouris, Dominique Spaeth, Luis Teixeira, Isabelle Tennevet, Cristian Villanueva, Benoit You, Johannes Ettl, Bernd Gerber, Oliver Hoffmann, Tjoung-Won Park-Simon, Mattea Reinisch, Joke Tio, Pauline Wimberger, Katalin Boer, Alberto Ballestrero, Giampaolo Bianchini, Laura Biganzoli, Roberto Bordonaro, Francesco Cognetti, Michelino De Laurentiis, Sabino De Placido, Valentina Guarneri, Filippo Montemurro, Giuseppe Naso, Armando Santoro, Claudio Zamagni, Seung-Jin Kim, Seigo Nakamura, Yee Soo Chae, Eun Kyung Cho, Kim Jee Hyun, Seock-Ah Im, Keun Seok Lee, Yeon Hee Park, Joo Hyuk Sohn, Tomasz Byrski, Tomasz Huzarski, Bozena Kukielka-Budny, Zbigniew Nowecki, Renata Szoszkiewicz, Rafal Tarnawski, Viktoria Dvornichenko, Fedor Moiseenko, Guzel Mukhametshina, Elena Poddubskaya, Ekaterina Popova, Anna Tarasova, Anna Vats, Bárbara Adamo, Raquel Andrés Conejero, Antonio Antón Torres, Judith Balmaña Gelpi, Nieves Díaz Fernández, Alejandro Falcón González, Juan Garcia, Isabel Lorenzo-Lorenzo, Fernando Moreno Antón, Marta Santisteban, Agostina Stradella, Chiun-Sheng Huang, Sercan Aksoy, Cagatay Arslan, Mehmet Artac, Adnan Aydiner, Ozgur Ozyilkan, Emel Sezer, Anne Armstrong, Sophie Barrett, Annabel Borley, Zoe Kemp, Caroline Michie, Mukesh Mukesh, Timothy Perren, Angela Swampillai, and Tammy Young

Subjects
0301 basic medicine, Oncology, Cancer Research, Receptor, ErbB-2, BRCA2 gene, Effectiveness, Piperazines, chemistry.chemical_compound, BRCA1 gene, 0302 clinical medicine, Breast cancer, Olaparib, ErbB-2, Germline mutation, Treatment outcome, Adjuvant, BRCA1 Protein, Middle Aged, Metastatic breast cancer, Progression-Free Survival, Chemotherapy, Adjuvant, 030220 oncology & carcinogenesis, Metastatic, Female, Receptor, Adult, medicine.medical_specialty, Anthracycline, Breast Neoplasms, Poly(ADP-ribose) Polymerase Inhibitors, 03 medical and health sciences, Young Adult, Progression-free survival, Aged, BRCA2 Protein, Germ-Line Mutation, Humans, Phthalazines, Internal medicine, medicine, Chemotherapy, Adverse effect, Taxane, business.industry, medicine.disease, Interim analysis, 030104 developmental biology, chemistry, business
Abstract

Background In the phase III OlympiAD trial, olaparib significantly increased progression-free survival (PFS) compared with chemotherapy of physician's choice in patients with germline BRCA-mutated (gBRCAm), human epidermal growth factor 2 (HER2)-negative metastatic breast cancer (mBC). The phase IIIb LUCY trial assessed the clinical effectiveness of olaparib in similar patients, in a setting reflecting clinical practice. Methods This open-label, single-arm trial of olaparib (300 mg, twice daily) enrolled patients with BRCAm, HER2-negative mBC who had received taxane and/or anthracycline in the (neo)adjuvant/metastatic setting and not more than two lines of prior chemotherapy for mBC. Patients with hormone receptor–positive mBC had progressed on at least one line of endocrine therapy in an adjuvant/metastatic setting and were unsuitable for further endocrine treatment. This interim analysis was planned after 160 PFS events. Results Of 563 patients screened, 252 patients with gBRCAm were enrolled and received at least one dose of olaparib. The median investigator-assessed PFS was 8.11 months (95% confidence interval [CI], 6.93–8.67; 166/252 events [65.9% maturity]). The investigator-assessed clinical response rate was 48.6%, and median time to first subsequent treatment or death was 9.66 months (95% CI, 8.67–11.14). The most common treatment-emergent adverse events (TEAEs; >20% patients) were nausea, anaemia, asthenia, vomiting and fatigue. Eleven patients (4.4%) discontinued treatment because of a TEAE. Grade 3 or higher TEAEs occurred in 64 patients (25.4%), including anaemia (33 patients; 13.1%). Conclusion Olaparib was clinically effective in patients with gBRCAm, HER2-negative mBC with safety outcomes consistent with previous findings. ClinicalTrials.gov identifier: NCT03286842 .

Published
2020

416. BLADE: Bayesian Log-normAl DEconvolution for enhanced in silico microdissection of bulk gene expression data

Author

Bárbara Andrade Barbosa, Saskia van Asten, Ji-won Oh, Arantza Fariña-Sarasqueta, Joanne Verheij, Frederike Dijk, Hanneke van Laarhoven, Bauke Ylstra, Juan Garcia-Vallejo, Mark van de Wiel, and Yongsoo Kim

Abstract

High-resolution deconvolution of bulk gene expression profiles is pivotal to characterize the complex cellular make-up of tissues, such as tumor microenvironment. Single-cell RNA-seq provides reliable prior knowledge for deconvolution, however, a comprehensive statistical model is required for efficient utilization due to the inherently variable nature of gene expression. We introduce BLADE (Bayesian Log-normAl Deconvolution), a comprehensive probabilistic framework to estimate both cellular make-up and gene expression profiles of each cell type in each sample. Unlike previous comprehensive statistical approaches, BLADE can handle >20 cell types thanks to the efficient variational inference. Throughout an intensive evaluation using >700 datasets, BLADE showed enhanced robustness against gene expression variability and better completeness than conventional methods, in particular to reconstruct gene expression profiles of each cell type. All-in-all, BLADE is a powerful tool to unravel heterogeneous cellular activity in complex biological systems based on standard bulk gene expression data.

Published
2020
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417. Safety and Diagnostic Yield of Transthoracic Needle Aspiration of the Lung in Elderly Patients

Author

Drew, Willey, Juan, Garcia-Saucedo, Fernando, Stancampiano, Michael G, Heckman, Zachary, Klopman, Andrea, Koralewski, Matthew, Crawford, and Margaret M, Johnson

Subjects
Aged, 80 and over, Male, Lung Neoplasms, Postoperative Complications, Risk Factors, Biopsy, Needle, Age Factors, Humans, Solitary Pulmonary Nodule, Female, Aged, Retrospective Studies
Abstract

Pulmonary nodules in elderly patients are commonly encountered in clinical practice. Tissue sampling with image guided transthoracic needle aspiration is often performed but may be complicated by pneumothorax or bleeding. To understand the outcomes of transthoracic needle aspiration in the elderly, we retrospectively reviewed outcomes of patients age 75 or greater in a single tertiary center.Four-hundred eleven patients age 75 or greater with a pulmonary nodule identified on computed tomography who underwent needle aspiration of the lung were studied. Diagnostic yield and procedural complications were assessed for each patient and subgroups analysis of those age 85 or greater was performed.Malignancy was confirmed in 70% of subjects and a benign diagnosis identified in 9%. Of the 411 patents, 203 (49.4%) experienced a complication; 150 patients (36.5%) developed a pneumothorax and 79 (19.2%) had bleeding. No patient required transfusion, experienced persistent air leak or massive hemoptysis, air embolism or death. Post procedural hospitalization was required in 36 patients (8.8%) with a median hospital stay of 2 days. No factors were identified to be associated with occurrence of a complication (all p ≥ 0.16) and complications were not increased in those 85 or greater.Our results suggest that in an elderly population, image guided needle aspiration of a pulmonary nodule provides diagnostic findings in most patients. Procedural complications following are not uncommon but the severity and long-term impact are limited. The occurrence of complications is similar in those age 75-84 and age 85 and older.

Published
2020

418. Cognitive Functioning and Cortical Brain Thickness in Acromegaly Patients: A Pilot study

Author

Marina Fernández-Andújar, Mario Gutiérrez-Bedmar, Francisco Alfaro-Rubio, Isabel García-García, Silvia Maraver-Selfa, José Ramón Ramos-Rodriguez, Inmaculada González-Molero, Núria Roé-Vellvé, Natalia García-Casares, and Juan Garcia-Arnes

Subjects
Oncology, medicine.medical_specialty, Pilot Projects, 030209 endocrinology & metabolism, Neuropsychological Tests, 03 medical and health sciences, Cognition, 0302 clinical medicine, Quality of life, Internal medicine, Acromegaly, Humans, Medicine, Depression (differential diagnoses), Glycemic, medicine.diagnostic_test, business.industry, Neuropsychology, Brain, Magnetic resonance imaging, General Medicine, medicine.disease, Psychiatry and Mental health, Clinical Psychology, Cross-Sectional Studies, Neuropsychology and Physiological Psychology, Pegvisomant, Quality of Life, business, 030217 neurology & neurosurgery, medicine.drug
Abstract

Objective Cognitive effects in acromegaly patients are poorly understood and the mechanisms involved are still unclear. The aim of this study was to evaluate the cognitive function, depression, and quality of life of acromegaly patients treated with pegvisomant versus somatostatin analogues (SRLs) and to analyze the effect of the different treatments on cognition and possible structural brain changes. Methods This cross-sectional study involved 23 acromegaly patients divided into two groups according to treatment modality: One group of 9 patients treated with pegvisomant and another group of 14 patients treated with SRLs. All participants underwent blood analysis, neuropsychological tests, depression tests, quality of life assessment, and 3-Tesla magnetic resonance imaging. Results We found no significant differences between groups in the neuropsychological tests, depression or quality of life; nor in the whole-brain cortical thickness. In the SRL group, the volume of the thalamus correlated positively with executive function, a correlation not found in the pegvisomant group. In addition, the pegvisomant group had significantly higher levels of insulin than the SRL group. Conclusions In conclusion, in this pilot study, the type of pharmacological treatment in patients with acromegaly and good glycemic control did not influence the cognitive function and cortical brain thickness. However, pegvisomant could play a neuroprotective role on the thalamus that will have to be demonstrated with larger samples in future studies.

Published
2020
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419. Bayesian analysis of the spin distribution of LIGO/Virgo black holes

Author

Ester Ruiz Morales, Jose Francisco Nuño Siles, Juan Garcia-Bellido, and UAM. Departamento de Física Teórica

Subjects
Astrophysics and Astronomy, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Astrophysics::High Energy Astrophysical Phenomena, gr-qc, Population, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, 01 natural sciences, General Relativity and Quantum Cosmology, Gravitational waves, Spin, Binary black hole, 0103 physical sciences, Prior probability, education, 010303 astronomy & astrophysics, Spin-½, Physics, education.field_of_study, Black hole binaries, Spins, 010308 nuclear & particles physics, Gravitational wave, General Relativity and Cosmology, Isotropy, Astrophysics::Instrumentation and Methods for Astrophysics, Física, Astronomy and Astrophysics, LIGO, Space and Planetary Science, astro-ph.CO, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Gravitational wave detection from binary black hole (BBH) inspirals has become routine thanks to the LIGO/Virgo interferometers. The nature of these black holes remains uncertain. We study here the spin distributions of LIGO/Virgo black holes from the first catalog GWTC-1 and the first four published BBH events from run O3. We compute the Bayes evidence for several independent priors: flat, isotropic, spin-aligned and anti-aligned. We find strong evidence for low spins in all of the cases, and significant evidence for small isotropic spins versus any other distribution. When considered as a homogeneous population of black holes, these results give support to the idea that LIGO/Virgo black holes are primordial, JGB and ERM thank the Theory Division for their generous hospitality during their Sabbatical at CERN in 2018, when this work originated. The authors acknowledge support from the Research Project PGC2018-094773-B-C32 (MINECO-FEDER, Spain) and the Centro de Excelencia Severo Ochoa Program, Spain SEV-2016-0597

Published
2020

420. Antidiabetic Drugs in Alzheimer's Disease and Mild Cognitive Impairment: A Systematic Review

Author

Mario Muñoz-Jiménez, Juan Garcia-Arnes, Natalia García-Casares, and Alí Zaarkti

Subjects
medicine.medical_specialty, Cognitive Neuroscience, medicine.medical_treatment, Cognitive functioning, 03 medical and health sciences, 0302 clinical medicine, Cognition, Alzheimer Disease, Diabetes mellitus, Internal medicine, medicine, Diabetes Mellitus, Humans, Hypoglycemic Agents, 030214 geriatrics, business.industry, Liraglutide, Insulin, Antidiabetic drugs, Mild cognitive impairment, medicine.disease, Metformin, Clinical trial, Psychiatry and Mental health, Regular insulin, Geriatrics and Gerontology, business, Pioglitazone, Alzheimer’s disease, 030217 neurology & neurosurgery, medicine.drug
Abstract

Introduction: Considering that Alzheimer’s disease (AD) and diabetes mellitus share pathophysiological features and AD remains with no cure, antidiabetic drugs like intranasal insulin, glitazones, metformin, and liraglutide are being tested as a potential treatment. Objective: The aim of this systematic review was to assess the efficacy of antidiabetic drugs in patients with AD, mild cognitive impairment (MCI), or subjective cognitive complaints (SCCs). Cognition was studied as the primary outcome and modulation of AD biomarkers, and imaging was also assessed as a secondary outcome. Methods: We conducted a search in the electronic databases PubMed/MEDLINE, EMBASE, and Scopus seeking clinical trials evaluating the effect on cognition of antidiabetic drugs in patients with AD, MCI, or SCCs. Results: A total of 23 articles were found eligible. Intranasal regular insulin improved verbal memory in most studies, especially in apoE4− patients, but results in other cognitive domains were unclear. Detemir improved cognition after 2 months of treatment, but it did not after 4 months. Pioglitazone improved cognition in diabetic patients with AD or MCI in 3 clinical trials, but it is controversial as 2 other studies did not show effect. Metformin and liraglutide showed promising results, but further research is needed as just 2 clinical trials involved each of these drugs. Almost all drugs tested were shown to modulate AD biomarkers and imaging. Conclusions: Intranasal insulin, pioglitazone, metformin, and liraglutide are promising drugs that could be useful in the treatment of AD. However, many questions remain to be answered in future studies, so no particular antidiabetic drug can currently be recommended to treat AD.

Published
2020

421. COVID-19 vaccines: the importance of transparency and fact-based education

Author

Juan Garcia Burgos, Zvi Teitelbaum, Joop M. A. van Gerven, Andrew J. Webb, Adam F. Cohen, H. Flore, Anthonius de Boer, Ron A. M. Foucher, Serge Cremers, Willem van Eden, Health Care Governance (HCG), and Virology

Subjects
Pharmacology, 2019-20 coronavirus outbreak, Clinical Trials as Topic, COVID-19 Vaccines, Coronavirus disease 2019 (COVID-19), business.industry, Immunization Programs, Information Dissemination, SARS-CoV-2, Severe acute respiratory syndrome coronavirus 2 (SARS-CoV-2), COVID-19, Public relations, Transparency (behavior), Mass Vaccination, Immunogenicity, Vaccine, Editorial, Drug Development, SDG 3 - Good Health and Well-being, Taverne, Animals, Humans, Mass vaccination, Pharmacology (medical), Business, Patient Safety
Published
2020

422. The host galaxies of 106 rapidly evolving transients discovered by the Dark Energy Survey

Author

Juan Garcia-Bellido, E. Bertin, C. Frohmaier, P. Wiseman, Josh Frieman, Douglas L. Tucker, Kyler Kuehn, Antonella Palmese, S. Everett, N. E. Sommer, J. Gschwend, M. Pursiainen, Lluís Galbany, M. A. G. Maia, A. R. Walker, G. Tarle, J. Carretero, M. Sako, Tamara M. Davis, Mark Sullivan, A. Carnero Rosell, D. L. Hollowood, S. Serrano, Anais Möller, David J. James, A. K. Romer, Richard Kessler, Daniel Scolnic, Peter Doel, Paul Martini, Pablo Fosalba, Marcos Lima, H. T. Diehl, Karl Glazebrook, K. Honscheid, V. Scarpine, C. Lidman, B. E. Tucker, Daniela Carollo, E. Swann, I. Sevilla-Noarbe, N. Kuropatkin, Sunayana Bhargava, M. E. C. Swanson, T. N. Varga, D. L. Burke, L. N. da Costa, Jennifer L. Marshall, T. M. C. Abbott, Ryan J. Foley, Claudia P. Gutiérrez, Felipe Menanteau, Samuel Hinton, M. Costanzi, David J. Brooks, G. Gutierrez, S. Allam, Robert A. Gruendl, Geraint F. Lewis, E. J. Sanchez, B. P. Thomas, J. Annis, Michel Aguena, F. Paz-Chinchón, Ramon Miquel, M. Smith, Daniel Gruen, Michael Schubnell, M. Childress, L. Kelsey, A. A. Plazas, M. Vincenzi, E. Suchyta, M. Carrasco Kind, Enrique Gaztanaga, 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), 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, European Commission, European Research Council, Ministerio de Ciencia, Innovación y Universidades (España), Agencia Estatal de Investigación (España), Ministerio de Economía y Competitividad (España), and Generalitat de Catalunya

Subjects
transients: supernovae, Software_OPERATINGSYSTEMS, ComputingMethodologies_SIMULATIONANDMODELING, abundances [Galaxies], Data_CODINGANDINFORMATIONTHEORY, Astrophysics, star formation [Galaxies], 01 natural sciences, Luminosity, Photometry (optics), 0103 physical sciences, Hardware_INTEGRATEDCIRCUITS, 010303 astronomy & astrophysics, Fast blue, [PHYS]Physics [physics], Physics, 010308 nuclear & particles physics, photometry [Galaxies], supernovae [Transients], Astronomy and Astrophysics, ComputerSystemsOrganization_PROCESSORARCHITECTURES, Galaxy, Redshift, galaxies: photometry, Stars, Supernova, Space and Planetary Science, galaxies: star formation, Dark energy, galaxies: abundances
Abstract

DES Collaboration: et al., Rapidly evolving transients (RETs), also termed fast blue optical transients, are a recently discovered group of astrophysical events that display rapid luminosity evolution. RETs typically rise to peak in less than 10 d and fade within 30, a time-scale unlikely to be compatible with the decay of Nickel-56 that drives conventional supernovae (SNe). Their peak luminosity spans a range of −15 < Mg < −22.5, with some events observed at redshifts greater than 1. Their evolution on fast time-scales has hindered high-quality follow-up observations, and thus their origin and explosion/emission mechanism remains unexplained. In this paper, we present the largest sample of RETs to date, comprising 106 objects discovered by the Dark Energy Survey, and perform the most comprehensive analysis of RET host galaxies. Using deep-stacked photometry and emission lines from OzDES spectroscopy, we derive stellar masses and star formation rates (SFRs) for 49 host galaxies, and metallicities ([O/H]) for 37. We find that RETs explode exclusively in star-forming galaxies and are thus likely associated with massive stars. Comparing RET hosts to samples of host galaxies of other explosive transients as well as field galaxies, we find that RETs prefer galaxies with high specific SFRs (〈log (sSFR)〉 ∼ −9.6), indicating a link to young stellar populations, similar to stripped-envelope SNe. RET hosts appear to show a lack of chemical enrichment, their metallicities akin to long-duration gamma-ray bursts and superluminous SN host galaxies (〈12 + log (O/H)〉 ∼ 9.4). There are no clear relationships between mass or SFR of the host galaxies and the peak magnitudes or decline rates of the transients themselves., We acknowledge support from STFC grant ST/R000506/1. MSm, MSu, and CPG acknowledge support from from the European Union’s 7th Framework Programme (EU/FP7) European Research Council (ERC) grant no. 615929. LG was funded by the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 839090. This work has been partially supported by the Spanish grant PGC2018-095317-B-C21 within the European Funds for Regional Development (FEDER). LK was supported by the Science and Technology Facilities Council (grant number ST/P006760/1) through the DISCnet Centre for Doctoral Training. 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 MINECO under grants AYA2015-71825, ESP2015-66861, FPA2015-68048, SEV-2016-0588, SEV2016-0597, 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 Ciencia e Tecnologia (INCT) e-Universe (CNPq grant 465376/2014-2)

Published
2020
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424. Studies of Charm Quark Diffusion inside Jets Using Pb-Pb and pp Collisions at sNN=5.02 TeV

Author

Artur Lobanov, Nathaniel Pastika, Y-J Lee, Valery Zhukov, Alexander Spiridonov, Daniele Pedrini, Benedikt Maier, Konrad Deiters, Kyle Tos, Ioannis Evangelou, Geonhee Oh, C. K. Mackay, Lisa Borgonovi, A. A. Bin Anuar, F. Mohamad Idris, Malte Backhaus, Gabriella Pugliese, I. Van Parijs, Nicholas Wardle, Tao Huang, Francesca Nessi-Tedaldi, G. B. Mohanty, Shirin Chenarani, Jozsef Molnar, Y. Ban, M. I. Nagy, Damir Lelas, Dajeong Jeon, Andrea Perrotta, Fuqiang Wang, Sergey Polikarpov, Justin Pilot, Johannes Schulz, Gregory Rakness, A. Baden, M. Barrio Luna, Kenichi Hatakeyama, Anna Woodard, Andreas Werner Jung, Chandiprasad Kar, A. García Alonso, Giacomo Sguazzoni, Tapomoy Guha Sarkar, Kevin Lannon, Petr Moisenz, G. Della Ricca, David Ja Cockerill, Wolfgang Lange, Erik Gottschalk, Guenakh Mitselmakher, S. Orfanelli, J. De Clercq, Roger Rusack, Marc Dejardin, Tielige Mengke, M. A. Bhat, C. S. Moon, Petr Levchenko, Javier Duarte, Andrea Delgado, Duncan Leggat, Brian L Winer, Mehmet Özgür Sahin, Donato Creanza, Marc Dobson, Heiner Tholen, Isa Dumanoglu, Davide Zuolo, Umberto Dosselli, M. Gola, Giacomo Ortona, J. Taylor, H. El Mamouni, P. Martinez Ruiz del Arbol, Dan Quach, Nikolai Golubev, Anadi Canepa, Dario Menasce, S. Kaplan, Joscha Knolle, A. Álvarez Fernández, Narumon Suwonjandee, C. Paus, Simranjit Singh Chhibra, Rylan Conway, Kun Shi, D. R. Claes, Marcel Rieger, Garrett Funk, Anders Ryd, Gavin Davies, Jean-Baptiste Sauvan, J. F. de Trocóniz, Eric Conte, Matthias Ulrich Mozer, David Barney, Aleksandra Lelek, Stephanie Beauceron, Joshua Kunkle, A. Morelos Pineda, Johannes Brandstetter, Johannes Hauk, Jordan Damgov, D. Di Croce, Peter Hansen, Kisung Lee, Basile Vermassen, Jay Mathew Lawhorn, Claude Amsler, Brent Yates, Ulrich Husemann, S. B. Oh, Alexander Malakhov, Gigi Rolandi, T. Boccali, Maurizio Pierini, M. L. Vesterbacka Olsson, Sergey Vavilov, M. Voutilainen, Fabio Monti, Günter Flügge, Qiao Xu, Danyyl Brzhechko, Daniel Gonzalez, P. A. Piroué, Andrew Carnes, Jordan Tucker, M. Naimuddin, Tyler Ruggles, Robert Clare, Patrizia Azzi, Claudio Caputo, Stefano Argiro, Laurent Favart, Cristian Pena, Thomas Reis, Martin Lipinski, Viatcheslav Stolin, David Cussans, Josef Hrubec, E. A. De Wolf, Salim Cerci, Wolfgang Funk, Yuta Takahashi, James Hirschauer, C. Oropeza Barrera, Sioni Summers, Sumit Keshri, Tengizi Toriashvili, S. Bhattacharya, D. Horvath, Rizki Syarif, Ia Iashvili, Mohsen Naseri, S. Di Guida, Giorgia Rauco, Nancy Marinelli, Bajrang Sutar, Marius Preuten, John N. Wood, Nils Faltermann, Duong Nguyen, Vladyslav Danilov, Dimitri Bourilkov, S. W. Cho, Andrew Whitbeck, Viktor Veszpremi, Abdulla Abdulsalam, Michael Seidel, I. Gonzalez Caballero, Shabnam Jabeen, T. Aushev, J. Lykken, Pasquale Musella, Yangyang Cheng, Kevin Mcdermott, Dmytro Kovalskyi, T. Weiler, V. Kutzner, Ulascan Sarica, Gyorgy Vesztergombi, Ali Harb, Thomas Hebbeker, Paul Lecoq, Frank Jm Geurts, Smarajit Karmakar, Arnaud Steen, Boaz Klima, Pavel Parygin, J. S. Kim, Michael Tytgat, David Lange, Robin Erbacher, Senta Greene, Fabio Colombo, Jean-Roch Vlimant, Brajesh C Choudhary, Paul David Luckey, Marco Trovato, Alexander Lanev, T. Kress, Susan Dittmer, Christopher Brainerd, Zhenbin Wu, Bhawna Gomber, Marcello Mannelli, Alexey Baskakov, A. De Roeck, A. J. Campbell, A. David, Ksenia Shchelina, Albert M. Sirunyan, Andrea Bocci, Georg Auzinger, M. Aldaya Martin, Harvey B Newman, Jeffrey Berryhill, J. D. Tapia Takaki, Melike Akbiyik, A. Kayis Topaksu, H. A. Salazar Ibarguen, Nicholas Mucia, Matthieu Marionneau, Mehmet Zeyrek, Christian Schwanenberger, Francesco Brivio, Marco Musich, K. Vellidis, E. Di Marco, Gaël Touquet, Chiara Amendola, A. Di Florio, Pirmin Berger, Tommaso Dorigo, Sandra Malvezzi, W. L. Prado Da Silva, Sébastien Viret, Frank Würthwein, Manas Maity, Alexi Mestvirishvili, Ulrich Goerlach, Joze Zobec, Massimo Casarsa, Steve Nahn, Marco Meschini, Paolo Capiluppi, James Rohlf, Carlos Avila, Sergei Bitioukov, Ricardo Eusebi, Nabin Poudyal, Sharon Hagopian, Ralf Ulrich, Juliette Alimena, E. J. Tonelli Manganote, Krzysztof Piotrzkowski, Ekaterina Kuznetsova, Dominick Olivito, A. De Wit, Frans Meijers, Pietro Faccioli, D. H. Kim, Alberto Zucchetta, V. Petrov, Jim Hanlon, D. Soldi, Jose Chinellato, Richard Cavanaugh, Anton Taurok, Guido Tonelli, Zeljko Antunovic, K. Hurtado Anampa, Jian Wang, Iasonas Topsis-Giotis, Kalyanmoy Chatterjee, Georgios Daskalakis, Mythra Varun Nemallapudi, Sergei Gninenko, J. C. Freeman, Petr Mandrik, M. Shi, Nicolas Filipovic, Senka Duric, Guler Karapinar, S. Petrushanko, S. Roy Chowdhury, Colin Jessop, M. Calderon De La Barca Sanchez, Matthias Kasemann, Paola Salvini, Edward Scott, Kristian Harder, Stefan Wayand, D. Cutts, Shao Min Tan, Ivan Reid, Christine Mclean, Anastasia Grebenyuk, G. Dissertori, Jason Kamin, Ijaz Ahmed, Konstantin Androsov, Mia Tosi, L. Romero, Prashant Shukla, André Rosowsky, Andrew Ivanov, Piergiulio Lenzi, Virgil E Barnes, Giuseppe Latino, Y. t. Duh, Matthew Kilpatrick, Debabrata Bhowmik, Adrian Perieanu, Alessandro Giassi, A. Meyer, Süleyman Durgut, Russell Richard Betts, Conor Henderson, Prasenjit Mal, Christina Snyder, Mykola Savitskyi, Plamen Iaydjiev, Vincenzo Innocente, Silvia Maselli, Ioannis Papadopoulos, Efstathios Paganis, R. Frühwirth, Erica Brondolin, Nataliia Kovalchuk, A. Di Crescenzo, Lalit Mohan Pant, Alexandre Zabi, Florian Beaudette, Asif Saddique, Daniel Arcaro, Marek Walczak, Andrea Gelmi, Matthias Schröder, A. Rossi, Michael Benjamin Andrews, Simone Paoletti, Suchandra Dutta, J. A. Murillo Quijada, Giulio Mandorli, Anne-Marie Magnan, Wagner Carvalho, Terhi Jarvinen, Greg Landsberg, Cécile Caillol, Sw. Banerjee, Kyungwook Nam, Manjit Kaur, Marino Missiroli, Dmitry Hits, Jorma Tuominiemi, Y. C. Yang, Ivan Pozdnyakov, Ruchi Chudasama, S. Sarkar, Marco Rovere, P. E. Karchin, David Yu, Marco Toliman Lucchini, Mauricio Thiel, Andreas Güth, Peter Timothy Cox, Michael Mulhearn, Hui Li, Salvatore My, T. A. Gómez Espinosa, James Dolen, Giuseppe Fasanella, Sung Keun Park, Atanu Modak, Bugra Bilin, Marco Cipriani, Peter Elmer, Konstantin Matchev, Stephan Albert Wiederkehr, F. M. Stober, J. J. Hollar, Jean-Marie Brom, Marcella Diemoz, M. Flechl, John Paul Chou, Brian Paul Padley, Nairit Sur, Jeremy Mans, I. D. Sandoval Gonzalez, Fatma Boran, Zainol Abidin Ibrahim, D. E. Pellett, S. Choi, P. D. Dauncey, A. Castro, Alessio Ghezzi, S. M. A. Ghiasi Shirazi, Valeria Botta, M. De Palma, V. Monaco, Thomas Esch, Vladimir Popov, Otman Charaf, Jacopo Pazzini, Aaron Dominguez, Z. Xu, Bora Akgun, Johannes Haller, L. V. Kardapoltsev, Anna Colaleo, Francesco Fiori, J. Seixas, Merve Ince, Dhanush Anil Hangal, Yildiray Komurcu, J. L. Dulemba, Luca Brianza, Bobak Hashemi, Tom Cornelis, Shivali Malhotra, Tanmay Mudholkar, Ennio Monteil, Aldo Penzo, Nicolas Tonon, Imad Baptiste Laktineh, Lucas Taylor, Matthew Citron, John J. Leonard, M. Fernandez, S. Somalwar, Pedrame Bargassa, Bekhzod S Yuldashev, G. De Lentdecker, Lin Wang, Marco Cuffiani, Oliver Buchmuller, Mariana Araujo, Freya Blekman, Giuseppe Zito, Ilse Krätschmer, B. Tali, David Michael Morse, G. Hamel de Monchenault, Aditee Rane, Etiennette Auffray, Maurizio Biasini, A. Yagil, Sinan Sagir, Marta Felcini, Kati Lassila-Perini, Y. Mohammed, G. Cucciati, Ádám Hunyadi, Wei Li, Pushpalatha C Bhat, Luigi Guiducci, Gregory R Snow, Jared Turkewitz, Igor Volobouev, Matteo Cremonesi, Nitish Dhingra, S. Fiorendi, Gregory Iles, D. Stolp, C. F. González Hernández, Ilya Kravchenko, Jeroen Hegeman, Alexis Pompili, Stephen Sanders, A. Escalante Del Valle, Joosep Pata, Petra Merkel, De Hua Zhu, Wei Xie, Rainer Wallny, Christian Schomakers, Vadim Oreshkin, Elena Voevodina, Ioannis Papakrivopoulos, Xavier Coubez, Fabrice Couderc, Maria Teresa Grippo, Amitabh Lath, Simon Kudella, Nikolay Voytishin, Anupam Sharma, Andrzej Pyskir, K. H. M. Kwok, Kira Burt, Giovanni Petrucciani, Zehui Zhang, Felicitas Pauss, Fabio Cossutti, Igor Katkov, Joachim Mnich, Egidio Longo, Cameron Bravo, Nikitas Loukas, Francesca Ricci-Tam, Andris Skuja, Sébastien Brochet, Fotios Ptochos, Ettore Focardi, Vallary Bhopatkar, John Rander, Angela Mehta, Igor Miagkov, Ivica Puljak, C. Barth, Andrius Juodagalvis, R. Vilar Cortabitarte, Mani Tripathi, Rachel Bartek, Marco Peruzzi, Andreas Künsken, Maria Toms, Piero Giorgio Verdini, Usama Hussain, Owen Rosser Long, J. Suarez Gonzalez, Hans Reithler, Ben Bylsma, Francesca Cavallari, Stephen Wimpenny, Henning Flacher, Samuel Bein, Daniel Spitzbart, Anatoli Zarubin, Roberto Tenchini, Konstantinos Theofilatos, Sandor Czellar, Nikolaos Manthos, Meng Xiao, P. Kontaxakis, Manuel Giffels, Christian Laner, Martin Grunewald, J. Piedra Gomez, Peter Robmann, Guo-Ming Chen, Menglei Sun, Arabella Martelli, Muhammad Ahmad, O. Zenaiev, James Wetzel, Tiziano Camporesi, Colin Bernet, Ivan Amos Cali, A. Carvalho Antunes De Oliveira, Jorge Chaves, Si Xie, Norbert Neumeister, Suman Bala Beri, Helena Bialkowska, Ugur Kiminsu, Martti Raidal, Laurent Thomas, Mark Derdzinski, Merve Nazlim Agaras, J. G. Li, Roberto Rossin, Andrey Popov, Warren Clarida, Dana Z. Anderson, Robert Stone, Jian Sun, S. Bheesette, Fabio Ravera, Cesare Calabria, M. Csanad, Federico Preiato, Oleg Prokofyev, Wolfram Erdmann, Artur Kalinowski, Jacobo Konigsberg, John Michael Marraffino, E. De La Cruz-Burelo, Kenneth Call, Nicola Amapane, Matteo Sani, Cesar Augusto Bernardes, Philip Baringer, Enrico Robutti, George Stephans, Ivan Marchesini, Maren Tabea Meinhard, Riccardo Bellan, Alexander Ershov, Andreas Psallidas, C. Vander Velde, R. Bhattacharya, E. Carrera Jarrin, Douglas Wright, Ketino Kaadze, Ayse Polatoz, Giles Strong, P. Van Hove, Alice Cocoros, Panagiotis Katsoulis, Austin Baty, Y. Musienko, M. C. Fouz, Rajat Gupta, Mara Senghi Soares, Serguei Ganjour, Christian Contreras-Campana, Dominik Nowatschin, E. W. Vaandering, S. Nandan, A. De Iorio, Pietro Vischia, B. McMaster, Fionn Ball, Pamela Klabbers, Fan Xia, Dietrich Liko, Mykhailo Dalchenko, Suresh C Tonwar, C. Martinez Rivero, Sylvie Braibant-Giacomelli, Jeffrey Roskes, Stefano Colafranceschi, C. Scharf, Siarhei Shulha, Francisco Matorras, John A Coughlan, Mohsan Waseem Ather, Anna Stakia, Sébastien Wertz, Andreas Nowack, Andrew Ackert, Silvia Taroni, Adel Terkulov, Paolo Gunnellini, Stephen Mrenna, Denys Lontkovskyi, Caglar Zorbilmez, Claudio Grandi, Andrey Demiyanov, R. Taus, Sébastien Gadrat, Mayda Velasco, Kai-yu Cheng, Louise Skinnari, Marco Alexander Harrendorf, Dmitry Philippov, Samuel Boren, Koushik Mandal, Fábio Lúcio Alves, Andrea Gozzelino, L. J. Gutay, David Curry, V. Andreev, Alexander Titterton, V. Re, André Holzner, J. M. Vizan Garcia, E. Palencia Cortezon, David J. Smith, C. Martin Perez, Tariq Aziz, Dave M Newbold, Vito Palladino, Nural Akchurin, Santeri Laurila, Hannu Siikonen, Victor Murzin, Sridhara Dasu, Emilio Meschi, Marc Weinberg, Juliet Ritchie Patterson, Francesco Fienga, Darien Wood, Jyothsna Rani Komaragiri, Frank Jensen, Raúl Iraq Rabadán-Trejo, Alexander Schmidt, Marco Zanetti, U. Bhawandeep, Roy Montalvo, Burin Asavapibhop, Xunwu Zuo, M. C. Duran-Osuna, Isabell-Alissandra Melzer-Pellmann, Nikola Godinovic, Altan Cakir, Jingyu Luo, Ayman Al-bataineh, Prafulla Kumar Behera, Matthew Nguyen, Paolo Meridiani, Vivian O'Dell, Riccardo Andrea Manzoni, P. C. Tiwari, Joao Varela, Leander Litov, Ernesto Migliore, Jean-Pierre Merlo, Marko Dragicevic, Kerstin Borras, Efe Yazgan, Hans-Jürgen Simonis, Luciano Orsini, Luca Pacher, Todd Adams, Andrew Wightman, Martina Malberti, Vladimir Korotkikh, Wit Busza, Giorgio Apollinari, Claire Shepherd-Themistocleous, Antonis Agapitos, Ulf Behrens, M. A. Shah, Anton Babaev, Joanne Cole, W. T. Lin, Shin-Shan Yu, Tae Jeong Kim, Dylan Hsu, Alberto Benvenuti, Christian Veelken, Thi Hien Doan, Daniel Denegri, Maria Agnese Ciocci, Maria Florencia Canelli, Fabrizio Ferro, J Martin Blanco, Wenxing Fang, Geoffrey Hall, William Mcbrayer, G. N. Kim, Georgios Tsipolitis, Raman Khurana, Yu. Andreev, Charles Mueller, Juan Garcia-Ferrero, Alexei Raspereza, Michael Murray, Deniz Poyraz, Jakob Salfeld-Nebgen, Kirti Ranjan, Milos Dordevic, Carsten Hensel, George Karathanasis, Shalhout Shalhout, Y. Choi, Salvatore Rappoccio, L. Kreczko, Loukas Gouskos, Nadir Daci, David Sheffield, Aron Soha, Brandon Allen, Simon Kurz, A. K. Virdi, A. Bat, Kunal Kothekar, Dustin Burns, Alexandros Attikis, Suneel Dutt, L. J. Sanchez Rosas, Eija Tuominen, Roberto Dell'Orso, J. W. Gary, Patrick Connor, Nicholas John Hadley, Jehad Mousa, W-S Hou, Karl Matthew Ecklund, Q. Li, Miaoyuan Liu, Tutanon Sinthuprasith, Emrah Tiras, Toyoko Orimoto, Nazar Bartosik, A. Rizzi, Maral Alyari, Bolek Wyslouch, Sanjay Padhi, S. Abu Zeid, M. Melo De Almeida, B. Chazin Quero, V. Rodríguez Bouza, Benjamin Mesic, F. Pandolfi, Markus Klute, Pedro G Mercadante, Thomas Ferbel, Teruki Kamon, Dmitry Elumakhov, James Buchanan, Hans-Christian Kaestli, Marta Ruspa, Jay Dittmann, Joel Goldstein, Urs Langenegger, R. Sharma, Luciano Ristori, Milena Misheva, Luigi Calligaris, Rishika Bhardwaj, Giovanna Selvaggi, Martino Dall'Osso, János Karancsi, Tai Sakuma, Kevin Deroover, Maksim Azarkin, Giacomo Fedi, Hallie Trauger, G. P. Van Onsem, Zaixing Mao, J. Alcaraz Maestre, Elizabeth Starling, Hartmut Stadie, Natascha Krammer, Adrian Byszuk, Basil Schneider, James Zabel, René Caspart, Daniel Abercrombie, Stepan Obraztsov, O. Gonzalez Lopez, Bradley Cox, Katja Klein, Olivér Surányi, Marvin Johnson, N. Woods, Anshul Kapoor, C. Neu, Sebastian Thüer, S. J. Qian, M. M. Defranchis, Matti J Kortelainen, Cheng-Chieh Peng, Thong Nguyen, Kevin Pedro, Sergei Baidali, Dooyeon Gyun, Gobinda Majumder, Giuseppe Barbagli, Crisostomo Sciacca, Maxim Goncharov, Salvatore Nuzzo, Sergey Troshin, Pawan Kumar Netrakanti, Gabor Istvan Veres, Alexandre Mertens, David D'Enterria, K. A. Ulmer, Vitalii Okhotnikov, G. Bagliesi, A. Richards, K. Ehataht, Marco Pieri, David Fehling, Ian R Tomalin, David Saltzberg, C. 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Kellogg, Borislav Pavlov, Vladimir Karjavine, Csaba Hajdu, Emyr Clement, C. Fallon, Mario Masciovecchio, Huilin Qu, James Letts, S. Tkaczyk, David Stuart, Alice Mignerey, A. Benecke, Evgenii Tarkovskii, Stefanos Leontsinis, Chayanit Asawatangtrakuldee, Vladimir Epshteyn, Ioanna Papavergou, David Sperka, Gaelle Boudoul, Wolfgang Waltenberger, Alexis Kalogeropoulos, Lovedeep Kaur Saini, Xin Chen, Teresa Rodrigo, H. Van Haevermaet, Sam Harper, Shuichi Kunori, Teresa Lenz, Laurent Mirabito, C. Beirão Da Cruz E Silva, Steven Lowette, Marius Teroerde, Georgia Karapostoli, D. A. Sanz Becerra, J. A. Nash, Elisabetta Gallo, Vincenzo Ciriolo, Tomasz Frueboes, G. Grenier, Nathan Kellams, Robin Aggleton, Ferhat Ozok, Prasanna Siddireddy, T. Geralis, Jaehyeok Yoo, Mateusz Zarucki, Antoni Shtipliyski, Erich Schmitz, Lutz Feld, Shahram Rahatlou, E. Ayala, Jasper Lauwers, Seth Cooper, S. Williamson, Wajid Ali Khan, Semra Turkcapar, Inna Kucher, Linda Finco, Ping Tan, Mingshui Chen, Tuure Tuuva, Matthias Komm, Arnab Purohit, Elizabeth Kennedy, Margaret Zientek, Unki Yang, Simona Cometti, Scott Thomas, Ozgun Kara, Daniel Gastler, Alain Givernaud, Gregor Mittag, S. W. Lee, Seth Moortgat, Jennifer Chu, J. H. Kim, P. Sphicas, Anindya Roy, Muhammad Waqas, Izaak Neutelings, Viktor Khristenko, J. D. Richman, Gaël Perrin, Umesh Joshi, Irina Vardanyan, Predrag Milenovic, Peter R Hobson, Kin Ho Lo, Predrag Cirkovic, Viola Sordini, Achim Geiser, Erika Garutti, E. Eskandari Tadavani, Sudarshan Paramesvaran, Victor Daniel Elvira, Alexander Morton, Javier Cuevas, Bilal Kiani, Alexander Snigirev, F. Hartmann, Stephane Cooperstein, S. Ragazzi, Marcello Abbrescia, Sanjay Kumar, Ali Celik, John Strologas, J. Fernandez Menendez, Charles Maguire, J. R. González Fernández, Giancarlo Mantovani, Carlo Battilana, Clemens Wöhrmann, Sezen Sekmen, Danila Tlisov, Yeonju Go, A. Vagnerini, Christophe Ochando, Francesco Santanastasio, Stoyan Stoynev, A. Sanchez-Hernandez, Tongguang Cheng, Charles Ferraioli, Z. Liu, Pooja Saxena, Sergo Jindariani, J. Schwandt, A. G. Stahl Leiton, Caleb Smith, Florian Michael Pitters, V. M. Ghete, John Bradmiller-Feld, John Hakala, Alexander Bylinkin, D. Kim, Milena Quittnat, A. M. Rossi, Daniel Teyssier, T. Lenzi, Victor Perelygin, Manisha Lohan, Alessandra Fanfani, J. Duarte Campderros, Frixos A Triantis, Andrew Askew, R. L. Lander, Gurpreet Singh, M. Olmedo Negrete, Miao Hu, Karl Gill, Paul Sheldon, Yuichi Kubota, Yacine Haddad, S. Sanchez Cruz, Mauro Menichelli, Tamás Álmos Vámi, A. Da Rold, Luca Perniè, Roland Horisberger, Georgios Mavromanolakis, Michele Arneodo, Elisa Manoni, S. Luo, Brieuc Francois, Thomas Madlener, G. F. Chen, Christopher Rogan, Nicola Bacchetta, Maximilian Heindl, A. Pérez-Calero Yzquierdo, Andreas Albert, Nicolas Chanon, Helena Malbouisson, Alex J. Barker, S. Lo Meo, Camelia Mironov, Benedikt Vormwald, Ilknur Hos, J. N. Butler, Genius Walia, Paolo Lariccia, Dmitry Sosnov, Alexander Savin, M. Finger, Chad Freer, Stefan Piperov, Caleb Fangmeier, D. R. Mendis, R. Loveless, Igor Vorobiev, Martin Delcourt, Alessio Magitteri, Francesco Fallavollita, Julie Managan Hogan, Byung-Sik Hong, Michael Hildreth, Panos A Razis, Steven R. Simon, John Gabriel Acosta, M. S. Meyer, Matthew Joyce, Laura Borrello, Paul Lujan, Anastasia Karavdina, T. W. Wang, Bożena Boimska, Kerem Cankocak, Harrison Prosper, Marta Baselga, Nadja Strobbe, Stephen Robert Wagner, Jean-Laurent Agram, Young Ho Shin, G. Paspalaki, Anthony Moeller, Sourav Dey, P. Priyanka, Alexander Dierlamm, I. Dremin, P. De Castro Manzano, Aristotelis Kyriakis, Michal Szleper, Roberto Chierici, Chia-Ming Kuo, P. Major, Nadia Pastrone, Ferenc Sikler, Mauro Verzetti, Mario Kadastik, Alexander Dermenev, Candan Dozen, C. Diez Pardos, Michael Wayne Arenton, Andrés G Delannoy, Christopher Hill, Sean Kalafut, Shalini Thakur, James John Brooke, Cédric Prieels, Dong Ho Moon, Adam Elwood, Sami Lehti, Adish Vartak, David Bertsche, Valentina Mariani, Martina Ressegotti, P. Schütze, Oleksii Turkot, Michele Selvaggi, O. Behnke, Gulsen Onengut, Viktor Matveev, Ivan Shvetsov, Igor Golutvin, Mircho Rodozov, Jennifer Ngadiuba, H. Lee, Carlo Civinini, Clemens Lange, Attila Racz, Roberta Arcidiacono, Christian Schnaible, Jonathan Fulcher, Anatoli Pashenkov, Avto Kharchilava, Mikhail Ignatenko, Jelena Luetic, Tapio Lampén, Claudia Cecchi, K. Sandeep, Santiago Folgueras, George Alverson, X. Y. Gao, Roman Kogler, Satoshi Hasegawa, Benjamin Kreis, A. Bodek, Oleksii Toldaiev, Norraphat Srimanobhas, Dermot Moran, Mark Pesaresi, Claudia Ciocca, S. Shmatov, F. Torres Da Silva De Araujo, Vineet Kumar, Andreas Hinzmann, and Marcin Konecki

Subjects
Nuclear reaction, Physics, Meson, Nuclear Theory, High Energy Physics::Phenomenology, Hadron, General Physics and Astronomy, Parton, Jet (particle physics), 01 natural sciences, Charm quark, Nuclear physics, 0103 physical sciences, High Energy Physics::Experiment, Production (computer science), Nuclear Experiment, 010306 general physics, Energy (signal processing)
Abstract

The first study of charm quark diffusion with respect to the jet axis in heavy ion collisions is presented. The measurement is performed using jets with p_{T}^{jet}>60 GeV/c and D^{0} mesons with p_{T}^{D}>4 GeV/c in lead-lead (Pb-Pb) and proton-proton (pp) collisions at a nucleon-nucleon center-of-mass energy of sqrt[s_{NN}]=5.02 TeV, recorded by the CMS detector at the LHC. The radial distribution of D^{0} mesons with respect to the jet axis is sensitive to the production mechanisms of the meson, as well as to the energy loss and diffusion processes undergone by its parent parton inside the strongly interacting medium produced in Pb-Pb collisions. When compared to Monte Carlo event generators, the radial distribution in pp collisions is found to be well described by pythia, while the slope of the distribution predicted by sherpa is steeper than that of the data. In Pb-Pb collisions, compared to the pp results, the D^{0} meson distribution for 4

Published
2020
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425. Discovery of a Candidate Binary Supermassive Black Hole in a Periodic Quasar from Circumbinary Accretion Variability

Author

David J. James, Yu Ching Chen, Pablo Fosalba, David J. Brooks, Keith Bechtol, G. Gutierrez, Karl Glazebrook, Tim Eifler, V. Scarpine, Santiago Serrano, Flavia Sobreira, H. Thomas Diehl, Josh Frieman, Santiago Avila, Xin Liu, Carlos E. Cunha, Juan de Vicente, Shantanu Desai, Peter Doel, Jennifer L. Marshall, Juan Garcia-Bellido, Felipe Menanteau, Aurelio Carnero Rosell, Daniel Gruen, Emmanuel Bertin, Enrique Gaztanaga, Gregory Tarle, Richard Kessler, Mathew Smith, Ramon Miquel, B. Flaugher, J. Carretero, Matias Carrasco Kind, Devon L. Hollowood, Tamara M. Davis, K. Honscheid, Vinu Vikram, Marcos Lima, Richard G. McMahon, Hengxiao Guo, E. J. Sanchez, Molly E. C. Swanson, E. Suchyta, J. Gschwend, Elisabeth Krause, August E. Evrard, Yue Shen, Francisco J. Castander, Manda Banerji, Luiz N. da Costa, Paul Martini, Marcio A. G. Maia, R. Chris Smith, Christopher R. Davis, A. Miguel Holgado, Will Hartley, Eric Morganson, Ben Hoyle, S. Allam, Robert A. Gruendl, Andres Plazas Malagon, Kyler Kuehn, Chris B. D'Andrea, Alistair R. Walker, Marcelle Soares-Santos, Michael Schubnell, Wei-Ting Liao, E. Buckley-Geer, James Annis, A. Roodman, UAM. Departamento de Física Teórica, 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), Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), Generalitat de Catalunya, European Commission, Australian Research Council, and Instituto Nacional de Ciência e Tecnologia (Brasil)

Subjects
Astrophysics, Surveys, 7. Clean energy, 01 natural sciences, high-redshift [Galaxies], Astrophysics::Solar and Stellar Astrophysics, 010303 astronomy & astrophysics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Data Release, Galaxies: Active, Dark Energy, nuclei [Galaxies], Astrophysics::Earth and Planetary Astrophysics, Astrophysics - High Energy Astrophysical Phenomena, Galaxy Mergers, Digital Sky Survey, Galaxies: Nuclei, Oscillations, active [Galaxies], QUASARES, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Gravitational-Waves, 0103 physical sciences, Galaxy formation and evolution, Quasars: General, Astrophysics::Galaxy Astrophysics, Supermassive black hole, 010308 nuclear & particles physics, Gravitational wave, Spectral Energy-Distributions, Física, Astronomy and Astrophysics, Quasar, general [Quasars], Black hole physics, Mass, Light curve, Galaxies: High-Redshift, Astrophysics - Astrophysics of Galaxies, Redshift, Black Hole Physics, 13. Climate action, Space and Planetary Science, Variable Quasars, Astrophysics of Galaxies (astro-ph.GA), Dark energy, Galactic Nuclei, Circumbinary planet, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

Binary supermassive black holes (BSBHs) are expected to be a generic byproduct from hierarchical galaxy formation. The final coalescence of BSBHs is thought to be the loudest gravitational wave (GW) siren, yet no confirmed BSBH is known in the GW-dominated regime. While periodic quasars have been proposed as BSBH candidates, the physical origin of the periodicity has been largely uncertain. Here, we report discovery of a periodicity (p = 1607 ± 7 d) at 99.95 per cent significance (with a global p value of ∼10-3 accounting for the look elsewhere effect) in the optical light curves of a redshift 1.53 quasar, SDSS J025214.67-002813.7. Combining archival Sloan Digital Sky Survey data with new, sensitive imaging from the Dark Energy Survey, the total ∼20-yr time baseline spans ∼4.6 cycles of the observed 4.4-yr (rest frame 1.7-yr) periodicity. The light curves are best fit by a bursty model predicted by hydrodynamic simulations of circumbinary accretion discs. The periodicity is likely caused by accretion rate modulation by a milli-parsec BSBH emitting GWs, dynamically coupled to the circumbinary accretion disc. A bursty hydrodynamic variability model is statistically preferred over a smooth, sinusoidal model expected from relativistic Doppler boost, a kinematic effect proposed for PG1302-102. Furthermore, the frequency dependence of the variability amplitudes disfavours Doppler boost, lending independent support to the circumbinary accretion variability hypothesis. Given our detection rate of one BSBH candidate from circumbinary accretion variability out of 625 quasars, it suggests that future large, sensitive synoptic surveys such as the Vera C. Rubin Observatory Legacy Survey of Space and Time may be able to detect hundreds to thousands of candidate BSBHs from circumbinary accretion with direct implications for Laser Interferometer Space Antenna., Liao, Wei-Ting, et al. DES Collaboration, 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 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 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 Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020, and the Brazilian Instituto Nacional de Ciênciae Tecnologia (INCT) e-Universe (CNPq grant 465376/2014-2).

Published
2020
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426. Hyperinflammation and Fibrosis in Severe COVID-19 Patients: Galectin-3, a Target Molecule to Consider

Author

Juan Garcia-Revilla, Tomas Deierborg, Jose Luis Venero, and Antonio Boza-Serrano

Subjects
lcsh:Immunologic diseases. Allergy, cytokine storm, fibrosis, galectin-3, COVID-19, biomarker, lcsh:RC581-607
Abstract

COVID-19 disease have become so far the most important sanitary crisis in the XXI century. In light of the events, any clinical resource should be considered to alleviate this crisis. Severe COVID-19 cases present a so-called cytokine storm as the most life-threatening symptom accompanied by lung fibrosis. Galectin-3 has been widely described as regulator of both processes. Hereby, we present compelling evidences on the potential role of galectin-3 in COVID-19 in the regulation of the inflammatory response, fibrosis and infection progression. Moreover, we provide a strong rationale of the utility of measuring plasma galectin-3 as a prognosis biomarker for COVID-19 patients and propose that inhibition of galectin-3 represents a feasible and promising new therapeutical approach.

Published
2020
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427. 22% Efficiency Inverted Perovskite Photovoltaic Cell Using Cation‐Doped Brookite TiO2 Top Buffer

Author

Kai Wang, Sen Zhang, Xiaowen Hu, Xiao-Fang Jiang, Guofu Zhou, Colton Sheehan, Chang Liu, Juan Garcia, Lingling Shui, Shashank Priya, and Zhiyong Zhang

Subjects
Fullerene, Materials science, General Chemical Engineering, General Physics and Astronomy, Medicine (miscellaneous), 02 engineering and technology, 010402 general chemistry, 01 natural sciences, Biochemistry, Genetics and Molecular Biology (miscellaneous), Buffer (optical fiber), law.invention, law, General Materials Science, lcsh:Science, Perovskite (structure), Brookite, business.industry, inverted perovskite solar cells, Photovoltaic system, Doping, General Engineering, 021001 nanoscience & nanotechnology, Cathode, 0104 chemical sciences, high efficiency, visual_art, visual_art.visual_art_medium, Optoelectronics, durability, Nanorod, lcsh:Q, interface engineering, 0210 nano-technology, business
Abstract

Simultaneously achieving high efficiency and high durability in perovskite solar cells is a critical step toward the commercialization of this technology. Inverted perovskite photovoltaic (IP‐PV) cells incorporating robust and low levelized‐cost‐of‐energy (LCOE) buffer layers are supposed to be a promising solution to this target. However, insufficient inventory of materials for back‐electrode buffers substantially limits the development of IP‐PV. Herein, a composite consisting of 1D cation‐doped TiO2 brookite nanorod (NR) embedded by 0D fullerene is investigated as a top modification buffer for IP‐PV. The cathode buffer is constructed by introducing fullerene to fill the interstitial space of the TiO2 NR matrix. Meanwhile, cations of transition metal Co or Fe are doped into the TiO2 NR to further tune the electronic property. Such a top buffer exhibits multifold advantages, including improved film uniformity, enhanced electron extraction and transfer ability, better energy level matching with perovskite, and stronger moisture resistance. Correspondingly, the resultant IP‐PV displays an efficiency exceeding 22% with a 22‐fold prolonged working lifetime. The strategy not only provides an essential addition to the material inventory for top electron buffers by introducing the 0D:1D composite concept, but also opens a new avenue to optimize perovskite PVs with desirable properties.

Published
2020

428. Weak lensing of Type Ia Supernovae from the Dark Energy Survey

Author

Anais Möller, E. Bertin, A. K. Romer, Samuel Hinton, J. Gschwend, G. Gutierrez, A. Roodman, David J. Brooks, Sunayana Bhargava, T. N. Varga, Peter Doel, M. Smith, H. T. Diehl, Ramon Miquel, David Bacon, Ofer Lahav, Jennifer L. Marshall, Daniel Gruen, Jack Elvin-Poole, David J. James, Marcelle Soares-Santos, Kyler Kuehn, Ryan J. Foley, Geraint F. Lewis, Daniel Scolnic, D. L. Burke, A. Carnero Rosell, A. R. Walker, G. Tarle, M. E. C. Swanson, Juan Garcia-Bellido, Dragan Huterer, V. Scarpine, E. Suchyta, B. Flaugher, Robert A. Gruendl, Karl Glazebrook, Felipe Menanteau, J. Annis, Daniela Carollo, M. Sako, D. W. Gerdes, Peter Melchior, C. Lidman, B. E. Tucker, D. L. Hollowood, J. Carretero, Michael Schubnell, Tamara M. Davis, S. Desai, Michel Aguena, K. Honscheid, S. Serrano, M. Costanzi, I. Sevilla-Noarbe, N. Kuropatkin, L. N. da Costa, Antonella Palmese, M. A. G. Maia, Salcedo Romero de Ávila, Jochen Weller, Marcos Lima, F. J. Castander, T. M. C. Abbott, E. J. Sanchez, Edward Macaulay, A. A. Plazas, N. E. Sommer, D. J. Brout, M. Carrasco Kind, Robert C. Nichol, Enrique Gaztanaga, Laboratoire de Physique de Clermont (LPC), Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), 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, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS), Macaulay, E., Bacon, D., Nichol, R. C., Davis, T. M., Elvin-Poole, J., Brout, D., Carollo, D., Glazebrook, K., Hinton, S. R., Lewis, G. F., Lidman, C., Möller, A., Sako, M., Scolnic, D., Smith, M., Sommer, N. E., Tucker, B. E., Abbott, T. M. C., Aguena, M., Annis, J., Avila, S., Bertin, E., Bhargava, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Castander, F. J., Costanzi, M., da Costa, L. N., Desai, S., Diehl, H. T., Doel, P., Flaugher, B., Foley, R. J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D. L., Honscheid, K., Huterer, D., James, D. J., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Palmese, A., Plazas, A. A., Romer, A. K., Roodman, A., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., Varga, T. N., Walker, A. R., Weller, J., and Des, Collaboration

Subjects
Cosmological parameter, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cosmological parameters, FOS: Physical sciences, Astrophysics, 01 natural sciences, cosmology: observations, Large-scale structure of the universe, Astrophysics - Cosmology and Nongalactic Astrophysics, 0103 physical sciences, cosmological parameters, 010303 astronomy & astrophysics, Weak gravitational lensing, STFC, Angular correlation function, Physics, 010308 nuclear & particles physics, RCUK, Astronomy and Astrophysics, Redshift, observations [cosmology], Supernova, Amplitude, Space and Planetary Science, Skewness, Dark energy, large-scale structure of the universe, ST/N000668/1, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], observation [cosmology]
Abstract

We consider the effects of weak gravitational lensing on observations of 196 spectroscopically confirmed Type Ia Supernovae (SNe Ia) from years 1 to 3 of the Dark Energy Survey (DES). We simultaneously measure both the angular correlation function and the non-Gaussian skewness caused by weak lensing. This approach has the advantage of being insensitive to the intrinsic dispersion of SNe Ia magnitudes. We model the amplitude of both effects as a function of $\sigma_8$, and find $\sigma_8 = 1.2^{+0.9}_{-0.8}$. We also apply our method to a subsample of 488 SNe from the Joint Light-curve Analysis (JLA) (chosen to match the redshift range we use for this work), and find $\sigma_8 = 0.8^{+1.1}_{-0.7}$. The comparable uncertainty in $\sigma_8$ between DES-SN and the larger number of SNe from JLA highlights the benefits of homogeneity of the DES-SN sample, and improvements in the calibration and data analysis., Comment: 10 pages, 7 figures, MNRAS

Published
2020
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429. Baseline haematology, biochemistry, blood gas values and health status of the Galapagos swallow-tailed gull (Creagrus furcatus)

Author

Gregory A. Lewbart, Juan Pablo Muñoz-Pérez, Carlos A. Valle, Catalina Ulloa, Alice Skehel, Britta Denise Hardesty, Cristina Regalado, Diane Deresienski, Ronald K. Passingham, and Juan Garcia

Subjects
0106 biological sciences, medicine.medical_specialty, Creagrus furcatus, Physiology, Zoology, Management, Monitoring, Policy and Law, 010603 evolutionary biology, 01 natural sciences, pCO2, Internal medicine, biology.animal, medicine, Nature and Landscape Conservation, geography, geography.geographical_feature_category, Hematology, biology, 010604 marine biology & hydrobiology, Ecological Modeling, Baseline (sea), Baseline data, biology.organism_classification, Blood chemistry, Archipelago, Seabird, Research Article
Abstract

The swallow-tailed gull, Creagrus furcatus, is a seabird endemic to the Galápagos archipelago. In general health, blood chemistry and haematology, parameters have not been published for this species. Blood analyses were run on samples drawn from 58 clinically healthy swallow-tailed gulls captured at Islote Pitt on San Cristóbal Island in July 2016 (28) and South Plaza Island in June 2017 (30). A point of care blood analyzer (iSTAT) was used in the field to obtain results for HCO3−, pH, pCO2, pO2, TCO2, anion gap, chloride, creatinine, glucose, haematocrit, haemoglobin, ionized calcium, potassium, sodium and urea nitrogen. A portable Lactate Plus™ analyzer was used to measure lactate. The baseline data reported is valuable for comparisons amongst different populations in the archipelago and to detect changes in health status of Galápagos swallow-tailed gulls.

Published
2020

430. Arginine deprivation alters microglial polarity and synergizes with radiation to eradicate non-arginine-auxotrophic glioblastoma tumors

Author

Nabil Hajji, Juan Garcia-Revilla, Manuel Sarmiento Soto, Richard Perryman, Jake Symington, Chad C. Quarles, Deborah R. Healey, Yijie Guo, Manuel Luis Orta-Vázquez, Santiago Mateos-Cordero, Khalid Shah, John Bomalaski, Giulio Anichini, Andreas G. Tzakos, Timothy Crook, Kevin O’Neill, Adrienne C. Scheck, Jose Luis Venero, Nelofer Syed, Brain Tumour Research Campaign, Brain Tumour Research, CRUK, European Commission, Convergence Science Centre (UK), Hellenic Foundation for Research and Innovation, Ministerio de Ciencia, Innovación y Universidades (España), Junta de Andalucía, Polaris Pharmaceuticals, Universidad de Sevilla. Departamento de Bioquímica y Biología Molecular, Universidad de Sevilla. Departamento de Biología Celular, European Commission (EC). Fondo Europeo de Desarrollo Regional (FEDER), National Strategic Reference Framework. (NSRF) E.U., Ministerio de Ciencia, Innovación y Universidades (MICINN). España, and Universidad de Sevilla

Subjects
Hydrolases, Immunology, MICROENVIRONMENT, Antineoplastic Agents, Therapeutics, Research & Experimental Medicine, METABOLISM, Argininosuccinate Synthase, Amino acid metabolism, Brain cancer, Arginine, Polyethylene Glycols, CONCOMITANT, Cell Line, Tumor, Humans, NITRIC-OXIDE SYNTHASE, 11 Medical and Health Sciences, Science & Technology, Nitric oxide, General Medicine, ADJUVANT TEMOZOLOMIDE, PEROXYNITRITE, CANCER, Medicine, Research & Experimental, Oncology, CELLS, SURVIVAL, Microglia, Glioblastoma, Life Sciences & Biomedicine, RADIOTHERAPY
Abstract

New approaches for the management of glioblastoma (GBM) are an urgent and unmet clinical need. Here, we illustrate that the efficacy of radiotherapy for GBM is strikingly potentiated by concomitant therapy with the arginine-depleting agent ADI-PEG20 in a non-arginine-auxotrophic cellular background (argininosuccinate synthetase 1 positive). Moreover, this combination led to durable and complete radiological and pathological response, with extended disease-free survival in an orthotopic immune-competent model of GBM, with no significant toxicity. ADI-PEG20 not only enhanced the cellular sensitivity of argininosuccinate synthetase 1-positive GBM to ionizing radiation by elevated production of nitric oxide (˙NO) and hence generation of cytotoxic peroxynitrites, but also promoted glioma-associated macrophage/microglial infiltration into tumors and turned their classical antiinflammatory (protumor) phenotype into a proinflammatory (antitumor) phenotype. Our results provide an effective, well-tolerated, and simple strategy to improve GBM treatment that merits consideration for early evaluation in clinical trials., This work was supported by the Brain Tumour Research Campaign (BTRC), Brain Tumour Research (BTR) CRUK Convergence Science Centre at The Institute of Cancer Research, London, and Imperial College London (C309/A31316) and the European Regional Development Fund (ERDF) under the Operational Program Epirus 2014-2020, NSRF 2014-2020 (project code 5033092, BIOPREDICTOR) and by the Hellenic Foundation for Research and Innovation (HFRI) under the “First call for HFRI research projects to support faculty members and researchers and the procurement of high-cost research equipment grant” (project code: 991, PROTECT). This research was also funded from grants by the Spanish Ministerio de Ciencia, Innovación y Universidades/FEDER/UE RTI2018-098645-B-100) and from Consejería de Economía y Conocimiento of Junta de Andalucía/FEDER/UE P18-RT-1372 and US-1264806. BTRC and BTR grants were awarded to NS and KON. JS was a recipient of CRUK Clinical Academic Training Programme. ADI-PEG20 was a gift from Polaris Pharmaceuticals Inc.

Published
2020

431. Measurement of $$\hbox {t}{\bar{\hbox {t}}}$$ normalised multi-differential cross sections in $${\text {p}}{\text {p}} $$ collisions at $$\sqrt{s}=13\,{\text {TeV}} $$, and simultaneous determination of the strong coupling strength, top quark pole mass, and parton distribution functions

Author

Gabriella Pugliese, I. Van Parijs, Pieter David, Olga Evdokimov, Junghwan Goh, Kevin Lannon, G. Della Ricca, Maryam Zeinali, Patrick Jarry, Benjamin Charles Radburn-Smith, Livio Fanò, B. Stieger, Sabino Meola, Roberto Covarelli, Sergio Cittolin, Kenyi Hurtado Anampa, Guenakh Mitselmakher, S. Zahid, S. Orfanelli, Kevin Nash, Gourab Saha, Valentina Dutta, Jared Sturdy, Kaya Tatar, A. Bornheim, Peisen Ma, Sandra S. Padula, Yiwen Wen, Paolo Vitulo, Maximilian Knut Kiesel, A. Di Crescenzo, Matthias Schröder, A. Rossi, W. Da Silva, Jordan Damgov, D. Di Croce, A. Giassi, Y. C. Yang, Peter Hansen, Kisung Lee, Basile Vermassen, K. Wong, Kyungwook Nam, Vukasin Milosevic, Nikkie Deelen, E. M. Da Costa, William J Spalding, Jay Roberts, Stefano Bianco, Brandon Chiarito, H. S. Chen, Yury Ivanov, Andre Sznajder, Serdal Damarseckin, Lalit Mohan Pant, Abdollah Mohammadi, Bobak Hashemi, Tom Cornelis, Julie Malcles, D. Spiga, Jay Mathew Lawhorn, Claude Amsler, Laurent Favart, Prakash Thapa, A. Rinkevicius, Olivier Davignon, Dmitri Konstantinov, Javier Martin Blanco, A. P. Singh, Yuri Gershtein, G. G. Da Silveira, Cristina Riccardi, Francois Lagarde, Gobinda Majumder, V. Lemaitre, Cristian Pena, Thomas Reis, Shivali Malhotra, A. Zucchetta, Felicitas Pauss, Tanmay Mudholkar, Ennio Monteil, Aldo Penzo, Nicolas Tonon, Boris Grynyov, Shengquan Tuo, Abhigyan Dasgupta, Zviad Tsamalaidze, Nikolai Skatchkov, Louis Antonelli, N. Zaganidis, Robert Hirosky, Martin Lipinski, Viatcheslav Stolin, Frank Würthwein, Francisco Yumiceva, Ritva Kinnunen, Celso Martinez Rivero, P. C. Tiwari, Gregor Kasieczka, Marco Meschini, A. Whitbeck, John J. Leonard, Jordi Duarte Campderros, Manas Maity, Petar Maksimovic, Thorsten Chwalek, Cecilia Elena Gerber, P. Das, Diego Beghin, Gian Michele Innocenti, I. Babounikau, A. Ranieri, Livia Soffi, R. B. Garg, Christopher Seez, Andrea García Alonso, Ada Solano, Alexi Mestvirishvili, Ulrich Goerlach, Angira Rastogi, Jane Nachtman, Y. Chao, Lesya Shchutska, Andrea Massironi, Matteo Cremonesi, Sergio F Novaes, Samet Lezki, Joze Zobec, Morgan Lethuillier, Yasar Onel, Piotr Traczyk, Steve Nahn, Rishi Patel, Candan Isik, L. Silvestris, M. A. B. Ali, Geng-Yuan Jeng, Austin Baty, Paolo Capiluppi, James Rohlf, Carlos Avila, Sergei Bitioukov, Markéta Jansová, Francesco Navarria, Juozas Vaitkus, Malte Backhaus, Jose F Benitez, Samuel Higginbotham, Nicholas Wardle, Tao Huang, N. Tosi, Isa Dumanoglu, Giacomo Sguazzoni, Alan Campbell, P. G. Verdini, Nitish Dhingra, S. Fiorendi, Ejt Manganote, Samuel Bein, Ricardo Eusebi, Paolo Giacomelli, Stephan Linn, Yu S. S., Marguerite Tonjes, Christopher George Tully, Has Ibarguen, Ignacio Redondo, Yurii Maravin, Alexander Belyaev, Dimitri Bourilkov, A. De Cosa, Hannes Sakulin, Tilman Rohe, Samila Muthumuni, E. Tarkovskii, Maciej Misiura, Hongfang Liu, G. Maggi, L. Viliani, Marius Preuten, John N. Wood, Daniel Spitzbart, David Mark Raymond, Olivier Bondu, E. O. Olaiya, Christophe Delaere, Alex Kamenev, Victor Kim, Willem Verbeke, Armando Lanaro, Sara Nabili, Gilvan Alves, P. M. R. del Arbol, Irene Bachiller, Cristina Biino, Ivan Mikulec, Francesco Micheli, Gul Gokbulut, Wenxing Fang, Geoffrey Hall, William Mcbrayer, G. N. Kim, Indara Suarez, Ajeeta Khatiwada, Claudio Campagnari, Teppo Mäenpää, R. Mankel, Wolfgang Lohmann, Sanjay Padhi, Maciej Górski, Nils Faltermann, Duong Nguyen, Vladimir Gavrilov, H. Sert, Vladyslav Danilov, Hongbo Liao, Aleko Khukhunaishvili, Nabin Poudyal, Sharon Hagopian, Ralf Ulrich, Juliette Alimena, Krzysztof Piotrzkowski, Ekaterina Kuznetsova, J. G. Li, MV Marono, Roberto Rossin, Siew Yan Hoh, Alexander Ershov, Andreas Psallidas, Jian Wang, S. W. Cho, Viktor Veszpremi, Sonaina Undleeb, F. Santanastasio, Filip Moortgat, J. D. T. Takaki, Konstantinos Kousouris, Arne Reimers, Joshua Bendavid, Nicanor Colino, Ketino Kaadze, Christian Contreras-Campana, E. W. Vaandering, André Holzner, Santeri Laurila, Faridah Mohamad Idris, Raúl Iraq Rabadán-Trejo, Alexander Schmidt, Nadir Daci, David Sheffield, Vincenzo Innocente, Ioannis Papadopoulos, Efstathios Paganis, R. Frühwirth, Erica Brondolin, K. W. Bell, Nataliia Kovalchuk, Suneel Dutt, Roberto Dell'Orso, Jesus Puerta Pelayo, J. W. Gary, Virgil E Barnes, Andrzej Novak, Sergey Troshin, Shabnam Jabeen, Thomas Reitenspiess, M. Bluj, David D'Enterria, B. R. Yates, Laura Dodd, Andrew Levin, C. Madrid, Daniel Bloch, Vivek Sharma, Anna Teresa Meneguzzo, Salvador Carrillo Moreno, Edgar Carrera Jarrin, Giuseppe Benedetto Cerati, Yen-Jie Lee, Stavros Mallios, Johannes Wittmann, James D. Olsen, Doga Gulhan, Louis Lyons, N. V. Krasnikov, Jaana Kristiina Heikkilä, Hugues Lattaud, Helio Nogima, Dhanush Anil Hangal, W. H. Smith, Alberto Orso Maria Iorio, Felice Pantaleo, Chanwook Hwang, Giovanni Petrucciani, Apichart Hortiangtham, M. G. Albrow, J. S. Lange, David Petyt, W. Van Doninck, Christina Reissel, Ryan Mueller, Hans Rykaczewski, Troy Mulholland, Yu G. B., James Castle, Seungkyu Ha, Daniele Fasanella, D. Green, Zhiming Wang, Torben Dreyer, Nikolay Tyurin, Panagiotis Kokkas, S. K. Pflitsch, Niels Dupont, Roumyana Hadjiiska, Igor Smirnov, C. Neu, Thong Nguyen, David Overton, Sang Il Pak, Roberto Sacchi, Patricia Rebello Teles, Vytautas Dudenas, Kerstin Hoepfner, R. Bhattacharya, Douglas Wright, Giacomo Fedi, Giles Strong, P. Van Hove, Alice Cocoros, Savvas Kyriacou, Denis Rathjens, Clemencia Mora Herrera, Panagiotis Katsoulis, F. T. D. S. De Araujo, R. M. Brown, Hannes Jung, Mark Saunders, O. Zenaiev, Martijn Mulders, Davide Zuolo, Marek Gruchala, Kevin Mcdermott, Dmytro Kovalskyi, V. Kutzner, Ali Harb, Frank Jm Geurts, Smarajit Karmakar, Lieselotte Moreels, Anton Stepennov, Ashley Parker, Mauro Donegà, Igor Bayshev, H. Keller, Stephen Mrenna, Denys Lontkovskyi, Konstantinos Manolopoulos, L. V. Kardapoltsev, Amitabh Lath, Simon Kudella, Cameron Bravo, Y. J. Mao, Chiara Mariotti, Houmani El Mamouni, Marco Monteno, Ohannes Kamer Köseyan, TT de Fatis, Alexander Dierlamm, Alessio Ghezzi, Johannes Haller, Christian Schomakers, A. Rose, S. Kaur, A. Bragagnolo, Weinan Si, Robert M Harris, Elliot Hughes, Jeremy Mans, Andrew Buccilli, Charles C. Richardson, James Bowen, Sergei Gleyzer, Ana Ovcharova, J. K. Lim, W. Ko, D. H. Miller, Mikhail Kirsanov, G. Iaselli, R. Cousins, M. A. Wadud, Giorgio Apollinari, Ulf Behrens, M. A. Shah, Tejinder Virdee, M. Jones, Camilla Galloni, M. Khakzad, Zhengcheng Tao, Gy L. Bencze, J. M. Hernandez, Edward Laird, Aurore Savoy-Navarro, Luca Mastrolorenzo, Vieri Candelise, Zainol Abidin Ibrahim, Gage Dezoort, D. E. Pellett, Konstantinos Theofilatos, Seth Conrad Zenz, Andrew Godshalk, Vincenzo Daponte, Daniele Marconi, Ted Kolberg, Muhammad Shoaib, Claude Charlot, Julia Thom, Finn Rebassoo, Juan Manuel Grados Luyando, Filippo Errico, Deepak Kumar Sahoo, F. Simonetto, Jean-Louis Faure, Philipp Millet, Vadim Oreshkin, Afiq Aizuddin Bin Anuar, Alexandre Zabi, Pedro José Fernández Manteca, Song-Ming Wang, Charles Mueller, Benjamin Mesic, Kamal Lamichhane, Mary Hadley, Martino Margoni, Sergio P Ratti, C. Barth, Andrius Juodagalvis, Volker Blobel, S. Choi, Michal Szleper, Roberto Chierici, Chia-Ming Kuo, J. Alexander, G. M. Bilei, Frank Chlebana, Sandor Czellar, Joshua Hardenbrook, A. Toropin, Kuntal Mondal, Giovanni Organtini, P. Kontaxakis, Manuel Giffels, Morgan Martin, Jian Sun, Kirika Uchida, Brian Francis, P. Van Mechelen, A. Muhammad, Teruki Kamon, Soon Gul Lee, James Buchanan, Maxim Pieters, A. Di Francesco, Alessio Boletti, Jie Zhang, Francesca Romana Cavallo, Ulrich Heintz, M. Kovac, Bjorn Burkle, P. Major, Alessia Saggio, Erhan Gülmez, Kaori Maeshima, Martin Erdmann, Piet Verwilligen, Pavel Bunin, Stefan Spanier, Andreas Hinzmann, Jpf Ramos, Boaz Klima, J. S. Kim, Michael Tytgat, David Lange, Brian Dorney, Robin Erbacher, Cristina Oropeza Barrera, Senta Greene, Artur Kalinowski, Viktor Savrin, Mitchell Wayne, Karol Bunkowski, Tanvi Wamorkar, Marco Zanetti, U. Bhawandeep, Guo-Ming Chen, Menglei Sun, A. Apyan, Arabella Martelli, Mariarosaria D'Alfonso, Mario Galanti, David Jonathan Hofman, Zoltan Szillasi, Paolo Checchia, A. Terkulov, John Almond, Shubham Pandey, Wei Shi, Andrew Beretvas, Otto Hindrichs, S. Mitra, Aashaq Shah, O. Rieger, Thomas Klijnsma, Mikhail Gavrilenko, W. S. Hou, Nadezda Chernyavskaya, Reddy Pratap Gandrajula, S. Bheesette, Andrey Uzunian, Neeti Parashar, Candan Dozen, Muhammad Ahmad, Suman Bala Beri, Helena Bialkowska, Andrew Wisecarver, W. T. Hung, P. Gras, Alexey Baskakov, C. West, W. Ji, Claudio Quaranta, Giuseppe Barbagli, Marcin Konecki, Artur Lobanov, Fabio Ravera, Maren Tabea Meinhard, Michael Wayne Arenton, Kerstin Borras, Simone Pigazzini, Sean Kalafut, Manfred Paulini, Pierluigi Bortignon, J. S. H. Lee, Tae Jeong Kim, Michael Murray, Jakob Salfeld-Nebgen, Kunal Kothekar, Dong-Chul Son, R. Yohay, Nur Zulaiha Jomhari, Klaus Rabbertz, Sebastiano Albergo, Lindsey Gray, Vivian O'Dell, Juska Pekkanen, Stephen Sanders, J. Rander, Joosep Pata, Colin Bernet, Nadia Pastrone, Francesca Cavallari, Alberto Belloni, Igor Lokhtin, Myriam Schönenberger, Marco Alexander Harrendorf, Dmitry Philippov, Andrew Hart, Demetrios Loukas, Erik Butz, Jan Kieseler, Georg Auzinger, Antonio Morelos Pineda, Giulia Negro, Harvey B Newman, Jeffrey Berryhill, S. Slabospitskii, James Keaveney, Patricia McBride, Krzysztof Doroba, Dylan Rankin, Andrew Brinkerhoff, Thomas Ferguson, Jose Flix, Sadia Khalil, Stefan Grünendahl, Didier Contardo, E. Voevodina, James John Brooke, Cédric Prieels, Nathaniel Pastika, Christopher Palmer, Melike Akbiyik, Alice Bean, Kyle Tos, Antonio Delgado Peris, Amedeo Staiano, Robert Schöfbeck, Ioannis Evangelou, C. K. Mackay, Ugo Gasparini, Veikko Karimäki, Nikola Godinovic, Hualin Mei, Lisa Borgonovi, Ernesto Migliore, Hans-Jürgen Simonis, Todd Adams, Andrew Wightman, Nazar Bartosik, Enrique Palencia Cortezon, A. Sanchez-Hernandez, Gabriel Madigan, Philip Harris, Noemi Beni, K. S. Lee, D. Krücker, Fábio Lúcio Alves, Efe Yazgan, Luciano Orsini, Luca Pacher, Stefano Belforte, Jan Eysermans, A. Venturi, Massimo Casarsa, Manuel Alejandro Segura Delgado, E. A. Yetkin, Ugur Kiminsu, P. Janot, Dario Soldi, Tobias Pook, Liliana Teodorescu, Jay Hauser, Matti J Kortelainen, Shervin Nourbakhsh, Wit Busza, Vyacheslav Valuev, Thomas Bergauer, Cheng-Chieh Peng, Rostyslav Shevchenko, Zachary Lesko, J. Seixas, Merve Ince, Attilio Santocchia, Jean Fay, Marvin Johnson, N. Woods, Sertac Ozturk, V. Veckalns, M. Della Negra, Javier Fernandez Menendez, Michael Planer, Maria Isabel Josa, P. Busson, Aaron Bundock, Katerina Lipka, Nicholas Eminizer, Daniele Pedrini, Abideh Jafari, Daniele Ruini, Alice Magnani, Altan Cakir, Paolo Meridiani, Aron Soha, Simon Kurz, A. Bat, Rogelio Reyes-Almanza, Nathan Mirman, Mia Tosi, L. Romero, Prashant Shukla, Martina Ressegotti, P. Schütze, Oleksii Turkot, J. R. G. Fernandez, P. Volkov, André Rosowsky, Andrew Ivanov, Benedikt Maier, Giacomo Bruno, Michele Selvaggi, E. Locci, Allison Reinsvold, Martin Kirakosyan, Tomas Hreus, Martti Raidal, O. Behnke, Gulsen Onengut, Viktor Matveev, Georgios Bakas, Clément Leloup, Konrad Deiters, Damir Lelas, Nabarun Dev, Johan Borg, S. Jain, Claire Shepherd-Themistocleous, Antonis Agapitos, O. Buchmuller, Andrés G Delannoy, Christopher Hill, Ren-Yuan Zhu, Pascal Vanlaer, Luciano Barone, F. Palla, Etiennette Auffray, Richard Breedon, Vasken Hagopian, G. M. Dallavalle, Michail Bachtis, Maurizio Biasini, Sergei Baidali, Bhargav Madhusudan Joshi, Dooyeon Gyun, Thi Hien Doan, Pamela Klabbers, Daniel Denegri, A. B. Meyer, Constantin Heidegger, R. Del Burgo, Vladimir Mossolov, Z. Zhang, Burin Asavapibhop, Giuseppe Fasanella, Sung Keun Park, Burak Bilki, M. Weber, Vladimir Andreev, Aruna Nayak, Nicolò Trevisani, G. B. Mohanty, H. Lee, GH de Monchenault, T. Boccali, Lfc Sierra, Gervasio Gomez, Elizabeth Starling, Nan Lu, Bugra Bilin, René Caspart, Gianluca Cerminara, Elisabetta Manca, Kati Lassila-Perini, Damir Devetak, Michele Bianco, M. Tadel, C. A. Carrillo Montoya, Eva Halkiadakis, A. Nikitenko, Isidro Gonzalez Caballero, M. A. Bhat, C. S. Moon, Silvia Goy Lopez, Zoltan Gecse, Matteo Presilla, Zeynep Demiragli, Marina Kolosova, W. E. Johns, Mariana Shopova, Yalcin Guler, Eric Christian Chabert, Frank Glege, K. Vellidis, Hartmut Stadie, Brian L Winer, L. S. Durkin, Souvik Das, Dajeong Jeon, Jasvinder A. Singh, Lorenzo Russo, Marc Dobson, A. Yagil, Sinan Sagir, Marta Felcini, Elizabeth Sexton-Kennedy, Clemens Lange, K. Sandeep, Prasant Kumar Rout, Nikitas Loukas, Matthias Wolf, Paolo Ronchese, Badder Marzocchi, Sanjay Kumar Swain, Marc M Baarmand, Daniel Salerno, Javier Duarte, Duncan Carlsmith, Márton Bartók, Y. F. Liu, Sarmad Masood Shaheen, Christoph Grab, Xuejun Wang, Marius Teroerde, Santiago Folgueras, George Alverson, X. Y. Gao, Roman Kogler, Satoshi Hasegawa, Benjamin Kreis, A. Bodek, Y. Skovpen, Oleksii Toldaiev, Mark Pesaresi, Riccardo Paramatti, Andrea Giammanco, Priyanka Kumari, Sean Flowers, Sandeep Bhowmik, Thiago Tomei, M. Rahmani, Natalia Lychkovskaya, Dipanwita Dutta, Meena Meena, Roger Wolf, Alexei Safonov, Heiner Tholen, S. Shmatov, Daniele Trocino, Silvia Maselli, Lev Dudko, Jeremy Andrea, A. Stahl, Sunil Bansal, Kenichi Hatakeyama, Natascha Krammer, Dong Ho Moon, Adam Elwood, Mani Tripathi, Rachel Bartek, A. Scribano, Marco Peruzzi, Usama Hussain, Owen Rosser Long, Timo Peltola, Shirin Chenarani, Joseph Heideman, James Bueghly, Matthew Nguyen, Marta Verweij, Hong Ni, Sebastian Thüer, S. J. Qian, Nicholas Smith, Petra Merkel, M. A. Mahmoud, Jingzhou Zhao, Rohan Bhandari, Vinay Hegde, David Zou, Andrey Korytov, P. Chang, D. Tsitsonis, Jorge Chaves, Si Xie, Pedro G Mercadante, Eduardo De Moraes Gregores, Jozsef Molnar, Valerio Re, W. A. T. Wan Abdullah, Ashfaq Ahmad, Michael Krohn, Jeremie Alexandre Merlin, Piotr Zalewski, Xinmei Niu, Hans-Christian Kaestli, Vitaly Smirnov, Jamal Rorie, Robert Stone, Jason Gilmore, Marco Paganoni, Henning Kirschenmann, Th. Müller, Don Lincoln, S. Sarkar, G. Zumerle, P. De CastroManzano, Lu R. S., Stephane Perries, T. A. GomezEspinosa, Carsten Heidemann, Costas Foudas, Jan Krolikowski, Luiz Mundim, C.-E. Wulz, Y. Ban, Michael Schmitt, P. E. Karchin, M. I. Nagy, Carlo Rovelli, Silvio Donato, W. T. Ford, Umberto Dosselli, M. Gola, Giacomo Ortona, J. Taylor, Riccardo Salvatico, Maurizio Pierini, Andrea Perrotta, Jose Monroy, Fuqiang Wang, Diego Matos Figueiredo, F. Gasparini, Justin Pilot, C. De OliveiraMartins, Markus Seidel, Petr Moisenz, David Ja Cockerill, Wolfgang Lange, Gianni Masetti, Erik Gottschalk, Vipin Bhatnagar, T. Liu, Jean-Charles Fontaine, Sami Lehti, Janos Erö, Warren Clarida, Dana Z. Anderson, Cesare Calabria, M. Csanad, Adish Vartak, Nicola Amapane, Georgia Karapostoli, David Cussans, Min-Hye Kim, A. C. Hernandez, Anton Dimitrov, David Bertsche, Raffaella Radogna, Valentina Mariani, Josef Hrubec, E. A. De Wolf, Salim Cerci, Ezio Torassa, Harry Cheung, Andrew Johnson, Ian Laflotte, C. Mills, Andreas Nowack, Vineet Kumar, Li Yuan, Andrea Gozzelino, I. De Bruyn, Reza Goldouzian, Mohd Nizam Yusli, W. De Boer, Jory Sonneveld, Hafeez R Hoorani, Ece Aşılar, K. F. Chen, Ilaria Vai, H. A. Weber, Gabriele Benelli, Peter Schleper, Dragos Velicanu, Qamar Hassan, Nuno Leonardo, A. Messineo, Zhen Hu, Zoltan Laszlo Trocsanyi, J. Conway, D. Del Re, Andrea Delgado, Jean-Baptiste Sauvan, Gigi Rolandi, Ashutosh Bhardwaj, M. C. De La Barca Sanchez, Duncan Leggat, Pedro Silva, I. R. Tomalin, S. Kaplan, Rebeca Gonzalez Suarez, Devdatta Majumder, Marco Verzocchi, Joscha Knolle, A. Triossi, Regina Demina, Vladimir Cherepanov, T. W. Wang, Dominique Gigi, Reyer Band, Raffaello D'Alessandro, Hasan Ogul, Julia Velkovska, Daniel John Karmgard, Manfred Jeitler, Sudha Ahuja, S. M. A. G. Shirazi, A. Kumar, Guillaume Bourgatte, Pushpalatha C Bhat, Halil Saka, Pietro Govoni, K. Wichmann, P. Kyberd, Renato Potenza, Pierluigi Zotto, Hwi Dong Yoo, Andrey Popov, Koushik Mandal, M. R. Adams, Giuseppe Codispoti, Mojtaba Mohammadi Najafabadi, L. J. Gutay, David Curry, M. Guchait, Robert Bainbridge, Fanbo Meng, Jhovanny Mejia Guisao, Caroline Collard, Ivan Shvetsov, S. Nuzzo, Igor Golutvin, Mircho Rodozov, S. Afanasiev, P. D. Dauncey, A. Castro, Anna Woodard, Petr Levchenko, Marco Costa, Nikolai Golubev, Patrizia Barria, Owen Baron, Vivekanand Jha, Steve Schnetzer, Saranya Ghosh, F. De Guio, Werner Lustermann, Andromachi Tsirou, Klaas Padeken, Alessandro Braghieri, Johannes Schulz, G. Tsipolitis, Somnath Choudhury, Juan Garcia-Ferrero, Alexei Raspereza, Pierluigi Paolucci, Thomas Schuh, Renato Campanini, Stefano Argiro, Gregory Rakness, C. Paus, Andrei Sobol, H. Bakhshiansohi, Gabriella Pasztor, D. R. Claes, Marcel Rieger, Anders Ryd, Gavin Davies, James Strait, Satyaki Chowdhury, Paul Baillon, A. P. C. Yzquierdo, Artur Apresyan, A. C. A. De Oliveira, Daniele Bonacorsi, Nicholas Haubrich, Wolfgang Funk, Sergey Vavilov, Aleksandr Iuzhakov, Yuta Takahashi, James Hirschauer, Ulascan Sarica, Christopher Brainerd, N. Raicevic, Lei Feng, L. Malgeri, Kamuran Dilsiz, Seema Bahinipati, Paolo Rumerio, Michael Reichmann, Lorenzo Uplegger, J. De Clercq, Sioni Summers, Mikko Voutilainen, Sumit Keshri, D. Horvath, Christian Autermann, Roger Rusack, Marc Dejardin, Mohsen Naseri, S. Di Guida, Guenter Eckerlin, Marc Besancon, Dinyar Rabady, Wolfram Dietrich Zeuner, Giorgia Rauco, Anton Babaev, Jennifer Ngadiuba, Armen Tumasyan, Nicola Bacchetta, Paula Eerola, Kenneth Bloom, Thomas Perry, M. De Mattia, M. Bharti, Dong Yu, Malgorzata Kazana, Sourabh Dube, Tielige Mengke, Attila Racz, Roberta Arcidiacono, Christian Schnaible, Jonathan Fulcher, Anatoli Pashenkov, Avto Kharchilava, Mikhail Ignatenko, Jelena Luetic, Tapio Lampén, Matthieu Marionneau, Mehmet Zeyrek, R. Loveless, Alessio Magitteri, M. Weinberg, Zhenbin Wu, Korbinian Schweiger, Anna Kropivnitskaya, P. de Barbaro, Bhawna Gomber, Kelly Beernaert, F. Zhang, Carlos Lourenco, Alexander Nehrkorn, Francesco Fienga, Andrzej Pyskir, Manoj Sharan, Igor Katkov, Byung-Sik Hong, Arsen Khvedelidze, R. Tenchini, Roy Montalvo, Joachim Mnich, John Perry Cumalat, Swagata Mukherjee, Alberto Benvenuti, Narumon Suwonjandee, Philip H Butler, Toni Sculac, Kun Shi, Rishika Bhardwaj, János Karancsi, Inkyu Park, H. Wei, Navid Rad, Zuhal Seyma Demiroglu, Andrew Carnes, Jordan Tucker, Yagya Raj Joshi, Philippe Bloch, Victor Golovtsov, Martina Vit, Najaf Amin, Grant Riley, Robert Fischer, Susan Gascon, Georgios Anagnostou, Melody A. Swartz, Maxwell Chertok, T. Aushev, Danek Kotlinski, Simone Gelli, A. Melo, Garrett Funk, Fabrizio Fabbri, Claudia Cecchi, Thomas Strebler, Marc Osherson, Gunther Roland, K. El Morabit, J. H. Kim, Lorenzo Bianchini, Marcello Mannelli, Christian Schwanenberger, Luca Perrozzi, Manfred Krammer, S. h. Seo, Hao Qiu, Kevin Sung, Peter Raics, Peicho Petkov, Leonardo Cristella, Francesco Brivio, Achille Petrilli, Chun-Hua Jiang, A. Volkov, M. Ramirez-Garcia, Michael Hildreth, M. S. Meyer, Plamen Iaydjiev, Denis Gelé, Catherine Schiber, Oscar Gonzalez Lopez, Mauro Emanuele Dinardo, Carmen Albajar, Sven Dildick, Maksym Titov, Daniel Klein, Herbert Rohringer, R. Cavanaugh, Alexander Lanev, Maria Agnese Ciocci, Maria Florencia Canelli, Fabrizio Ferro, Federico Ferri, Gordon H. Hanson, Thomas Ferbel, J. F. de Trocóniz, R. Bi, R. Di Maria, Mykola Savitskyi, G. Oh, Alexis Fagot, D. Creanza, C. E. Flores, Marta Ruspa, Stepan Obraztsov, Nhan Viet Tran, T. Kress, Susan Dittmer, Kalyanmoy Chatterjee, Georgios Daskalakis, Alessandra Romero, Valeria Botta, M. De Palma, Daniel Gonzalez, P. A. Piroué, Thomas Esch, Raffaele Gerosa, Alexander Ledovskoy, Vincent J Smith, Sergei Gninenko, Konstanty Sumorok, Semiray Girgis, J. C. Freeman, Petr Mandrik, M. Shi, Nicolas Filipovic, Alberto Santoro, Senka Duric, Guler Karapinar, Christof Roland, G. 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Dulemba, M. Fernandez, S. Somalwar, Pedrame Bargassa, Nikolay Voytishin, K. H. M. Kwok, Kira Burt, Stefano Colafranceschi, C. Scharf, Siarhei Shulha, A. Di Mattia, Paolo Gunnellini, Juliet Ritchie Patterson, Joao Varela, Leander Litov, Jean-Pierre Merlo, L. M. H. Guativa, J. M. V. Garcia, Joanne Cole, A. K. Virdi, Eija Tuominen, Luigi Fiore, Patrick Connor, Daniel Abercrombie, Gabor Istvan Veres, Sarah Catherine Eno, Jan-Frederik Schulte, Till Arndt, A. Kyriakis, Hugues Brun, Pieter Everaerts, J. Y. Han, Titas Roy, Alexx Perloff, Roman Ryutin, Federica Primavera, Roberto Carlin, Pierre Depasse, Vyacheslav Klyukhin, M. Van De Klundert, Sören Erdweg, Luisa Benussi, Richard B. Lipton, Kurt Jung, A. Baden, Dan Quach, I. Yu, Rylan Conway, Matthias Ulrich Mozer, Johannes Brandstetter, Evan Ranken, Alexander Malakhov, Qiao Xu, Danyyl Brzhechko, M. Naimuddin, Tyler Ruggles, A. Tricomi, Robert Clare, Cristina Martin Perez, Patrizia Azzi, Thomas Hebbeker, Paul Lecoq, A. De Roeck, A. David, Ksenia Shchelina, Albert M. Sirunyan, E. Di Marco, Gaël Touquet, J. S. Gonzalez, Chiara Amendola, A. Di Florio, A. De Wit, Frans Meijers, Edward Scott, D. Damiani, and Mikhail Danilov

Subjects
Quantum chromodynamics, Coupling constant, Physics, Top quark, Particle physics, Physics and Astronomy (miscellaneous), 010308 nuclear & particles physics, 01 natural sciences, Gluon, Distribution function, 0103 physical sciences, Invariant mass, Rapidity, 010306 general physics, Engineering (miscellaneous), Lepton
Abstract

Normalised multi-differential cross sections for top quark pair ($$\hbox {t}{\bar{\hbox {t}}}$$tt¯) production are measured in proton-proton collisions at a centre-of-mass energy of 13$$\,{\text {TeV}}$$TeV using events containing two oppositely charged leptons. The analysed data were recorded with the CMS detector in 2016 and correspond to an integrated luminosity of $$35.9{\,{\text {fb}}^{-1}} $$35.9fb-1. The double-differential $$\hbox {t}{\bar{\hbox {t}}}$$tt¯ cross section is measured as a function of the kinematic properties of the top quark and of the $$\hbox {t}{\bar{\hbox {t}}}$$tt¯ system at parton level in the full phase space. A triple-differential measurement is performed as a function of the invariant mass and rapidity of the $$\hbox {t}{\bar{\hbox {t}}}$$tt¯ system and the multiplicity of additional jets at particle level. The data are compared to predictions of Monte Carlo event generators that complement next-to-leading-order (NLO) quantum chromodynamics (QCD) calculations with parton showers. Together with a fixed-order NLO QCD calculation, the triple-differential measurement is used to extract values of the strong coupling strength $$\alpha _{S}$$αS and the top quark pole mass ($$m_{{\text {t}}}^{{\text {pole}}}$$mtpole) using several sets of parton distribution functions (PDFs). The measurement of $$m_{{\text {t}}}^{{\text {pole}}}$$mtpole exploits the sensitivity of the $$\hbox {t}{\bar{\hbox {t}}}$$tt¯ invariant mass distribution to $$m_{{\text {t}}}^{{\text {pole}}}$$mtpole near the production threshold. Furthermore, a simultaneous fit of the PDFs, $$\alpha _{S}$$αS, and $$m_{{\text {t}}}^{{\text {pole}}}$$mtpole is performed at NLO, demonstrating that the new data have significant impact on the gluon PDF, and at the same time allow an accurate determination of $$\alpha _{S}$$αS and $$m_{{\text {t}}}^{{\text {pole}}}$$mtpole. The values $$\alpha _{S}(m_{{\text {Z}}}) = 0.1135{}^{+0.0021}_{-0.0017}$$αS(mZ)=0.1135-0.0017+0.0021 and $$m_{{\text {t}}}^{{\text {pole}}} = 170.5 \pm 0.8 \,{\text {GeV}} $$mtpole=170.5±0.8GeV are extracted, which account for experimental and theoretical uncertainties, the latter being estimated from NLO scale variations. Possible effects from Coulomb and soft-gluon resummation near the $$\hbox {t}{\bar{\hbox {t}}}$$tt¯ production threshold are neglected in these parameter extractions. A rough estimate of these effects indicates an expected correction of $$m_{{\text {t}}}^{{\text {pole}}}$$mtpole of the order of $$+1 \,{\text {GeV}} $$+1GeV, which can be regarded as additional theoretical uncertainty in the current $$m_{{\text {t}}}^{{\text {pole}}}$$mtpole extraction.

Published
2020
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432. Measurement of prompt ψ(2S) production cross sections in proton–lead and proton–proton collisions at sNN=5.02TeV

Author

Benedikt Maier, Matti J Kortelainen, Cheng-Chieh Peng, Konrad Deiters, Dooyeon Gyun, Gobinda Majumder, Christine Mclean, Shirin Chenarani, Diego Matos Figueiredo, Maryam Zeinali, Patrick Jarry, Benjamin Charles Radburn-Smith, Jozsef Molnar, Valerio Re, Kevin Nash, Valentina Dutta, Marco Verzocchi, Fanbo Meng, Jhovanny Mejia Guisao, Caroline Collard, Stefano Ragazzi, Jane Nachtman, Sergio F Novaes, Samet Lezki, Georgios Anagnostou, Melody A. Swartz, Maxwell Chertok, Danek Kotlinski, Simone Gelli, Denis Gelé, Chang-Seong Moon, Martin Flechl, Nikkie Deelen, Prakash Thapa, Morgan Lethuillier, Yasar Onel, Mauro Emanuele Dinardo, Carmen Albajar, Sven Dildick, Jian Wang, Nhan Viet Tran, Mohammad Abrar Wadud, Christof Roland, Alexis Pompili, Iasonas Topsis-Giotis, Alexander Toropin, Jesus Puerta Pelayo, David Colling, Louie Corpe, Stephen Wimpenny, Henning Flacher, Olivier Davignon, Dmitri Konstantinov, Javier Martin Blanco, Francisco Yumiceva, Ritva Kinnunen, Nikolaos Manthos, Natale Demaria, Amina Zghiche, Christian Laner, Martin Grunewald, Emily MacDonald, Ignacio Redondo, Benjamin Stieger, Hyun-Chul Kim, Virgil E Barnes, Olivér Surányi, Olena Karacheban, Cristóvão Beirão Da Cruz E Silva, Andrew Gilbert, Yurii Maravin, Vladimir Gavrilov, Hongbo Liao, Aleko Khukhunaishvili, Sonaina Undleeb, Rostyslav Shevchenko, Sudeshna Banerjee, Vladimir Andreev, Ramandeep Kumar, Aruna Nayak, Michael Plagge, Alessio Ghezzi, Luigi Benussi, Gouranga Kole, Bruno Galinhas, Irving Daniel Sandoval Gonzalez, Ravi Janjam, Siddharth Narayanan, Anton Karneyeu, Leonard Apanasevich, Weinan Si, Jochen Schieck, Petar Maksimovic, Ridhi Chawla, Patrick Janot, Charalambos Nicolaou, Niki Saoulidou, Zhengcheng Tao, Sercan Sen, Andre Govinda Stahl Leiton, Gervasio Gomez, Zhenyu Chen, Federico Preiato, Oleg Prokofyev, Wolfram Erdmann, Nicolo Cartiglia, Thorsten Chwalek, Matthew Carver, Meenakshi Narain, Geoffrey Smith, Johannes Haller, Mirena Ivova Paneva, Markus Friedl, Rajat Gupta, Mara Senghi Soares, Serguei Ganjour, Silvia Taroni, Thomas Eichhorn, Mar Barrio Luna, Alessandro Thea, Cristina Fernandez Bedoya, Isabel Pedraza, Sunil Somalwar, Christian Schomakers, Vadim Oreshkin, Archana Sharma, Daniel Salerno, Stephen Sanders, Wesley H Smith, Rohan Bhandari, Vinay Hegde, Saptaparna Bhattacharya, David Zou, Andrey Korytov, Hannes Jung, Alexander Zhokin, Juan Alcaraz Maestre, Ahmad Borzou, Yi Chen, Saswati Nandan, Willi Bertl, Geng-Yuan Jeng, Irene Bachiller, P. 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Richardson, James Bowen, Daniele Spiga, Piotr Traczyk, David Jonathan Hofman, Giles Strong, Shubham Pandey, Wei Shi, Andrea Castro, Thomas Klijnsma, Stanislav Lisniak, Nadezda Chernyavskaya, Juska Pekkanen, Manuel Alejandro Segura Delgado, Giacomo Bruno, Manuel Calderon De La Barca Sanchez, Tomas Hreus, Damir Devetak, Michele Bianco, Rainer Mankel, Mariana Shopova, Eric Christian Chabert, Sean Flowers, Sandeep Bhowmik, Thiago Tomei, Julie Malcles, Fengwangdong Zhang, Yi-ting Duh, Boris Grynyov, Shengquan Tuo, Abhigyan Dasgupta, Zviad Tsamalaidze, Louis Antonelli, Michael Albrow, Hamed Bakhshiansohi, Antonio Morelos Pineda, Stephan Linn, Marguerite Tonjes, Olivier Bondu, Christophe Delaere, Jose Monroy, Victor Kim, Willem Verbeke, Armando Lanaro, Daniel Bloch, Edgar Carrera Jarrin, Giuseppe Benedetto Cerati, Stavros Mallios, Johannes Wittmann, James D. Olsen, Aobo Zhang, Xuyang Gao, J. S. Lange, Clemencia Mora Herrera, Lieselotte Moreels, German Martinez, Giannis Flouris, Cristina Botta, Georg Sieber, Viesturs Veckalns, Arnd Meyer, Dario Bisello, Jiyeon Han, Yu-Hsiang Chang, David Stickland, Daniel Pitzl, Joaquin Emilo Siado, Maksat Haytmyradov, Paolo Montagna, Othmane Bouhali, Carlos Erice, David Mason, Luigi Moroni, Luca Lista, Michael Wang, James G Branson, Jesus Marco, Sebastian Baur, David Krofcheck, Jonathan Hollar, Willis Lin, Anirban Saha, Andrew Evans, Ekaterina Avdeeva, Markus Merschmeyer, Arie Bodek, Eduardo Coelho, Ozlem Kaya, Sevil Salur, Wai Ting Hung, and Daniele Pedrini

Subjects
Physics, Nuclear and High Energy Physics, Large Hadron Collider, Meson, Proton, 010308 nuclear & particles physics, Nuclear Theory, Quarkonium, 01 natural sciences, Nuclear physics, Excited state, 0103 physical sciences, Quark–gluon plasma, High Energy Physics::Experiment, Rapidity, Nuclear Experiment, 010306 general physics, Ground state
Abstract

Measurements of prompt psi(2S) meson production cross sections in proton-lead (pPb) and proton-proton (pp) collisions at a nucleon-nucleon center-of-mass energy of root s(NN) = 5.02 TeV are reported. The results are based on pPb and pp data collected by the CMS experiment at the LHC, corresponding to integrated luminosities of 34.6 nb(-1) and 28.0 pb(-1), respectively. The nuclear modification factor R-pPb is measured for prompt psi(2S) in the transverse momentum range 4 < p(T) < 30 GeV/c and the center-of-mass rapidity range -2.4 < y(CM) < 1.93. The results on psi(2S) R-pPb are compared to the corresponding modification factor for prompt J/psi mesons. The results point to different nuclear effects at play in the production of the excited charmonium state compared to the ground state, in the region of backward rapidity and for PT < 10 GeV/c. (C) 2019 The Author. Published by Elsevier B.V.

Published
2019
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433. Search for supersymmetric partners of electrons and muons in proton–proton collisions at s=13TeV

Author

Zheng Wang, Wajid Ali Khan, Edy Ayala, Christopher Madrid, Emanuela Barberis, Wim De Boer, Abhisek Datta, Inna Kucher, Aysen Tatarinov, Jian Wang, Iasonas Topsis-Giotis, Alexander Toropin, Jesus Puerta Pelayo, Manuel Franco Sevilla, Tariq Aziz, Dave M Newbold, Marko Dragicevic, Tiziano Rovelli, Michal Bluj, Ping Tan, Willard Johns, Jian Sun, Artur Kalinowski, Avraham Yagil, Andrey Marinov, Francesca Cenna, Tomasz Frueboes, Nicola De Filippis, Monika Bharti, Alberto Ruiz-Jimeno, Gabriel Ramirez-Sanchez, Alessandro Di Mattia, Virgil E Barnes, Junho Kim, Michael Dittmar, George Karathanasis, Shalhout Shalhout, Steven Kaplan, Tuure Tuuva, Giuliana Galati, Brandon Allen, Dustin Burns, Jarne De Clercq, Joona Havukainen, Robert Cousins, Elizabeth Kennedy, Margaret Zientek, Unki Yang, Didar Dobur, Alessio Ghezzi, Sangeun Lee, Ozgun Kara, Marco Alexander Harrendorf, Nicole Ruckstuhl, Dmitry Philippov, Fábio Lúcio Alves, Seh Wook Lee, Austin Ball, Aleksandar Aleksandrov, Jacob Linacre, Ramkrishna Sharma, Urs Langenegger, Martino Dall'Osso, Vladimir Blinov, Nathaniel Odell, Daniel Gastler, Srinidhi Bheesette, Zaixing Mao, Yongbin Feng, Bernard Ille, Dustin Anderson, Juan Suarez Gonzalez, Dinko Ferencek, Johannes Haller, Christian Schomakers, Giovanni Franzoni, Zhangqier Wang, Alain Givernaud, Seth Moortgat, Carmen Diez Pardos, Frank Hartmann, Luciano Orsini, Evrim Ersin Kangal, Ashok Kumar, Ta-Yung Ling, Alessandro Montanari, Adrian Byszuk, Luca Pacher, Vasile Mihai Ghete, Claire Shepherd-Themistocleous, Antonis Agapitos, Thi Hien Doan, Luc Pape, Vassili Kachanov, Sanjeev Kumar, Crisostomo Sciacca, Moritz Guthoff, Marc Weber, Rafael Teixeira De Lima, Metin Yalvac, Stephan Lammel, Tagir Aushev, Muhammad Waqas, Hugo Delannoy, Daniel Noonan, Vadim Oreshkin, Julie Malcles, Fengwangdong Zhang, Salim Cerci, Olaf Behnke, Mia Tosi, Prashant Shukla, André Rosowsky, Andrew Ivanov, Krishna Thapa, Rachael Bucci, Maxim Goncharov, Richard D Field, Marco Pieri, Francesco Costanza, David Fehling, Izaak Neutelings, Predrag Milenovic, Evgueni Vlasov, Karl Ehataht, Peter R Hobson, Enrico Robutti, Ian R Tomalin, David Saltzberg, José David Ruiz Alvarez, Daniel Denegri, Kurtis F Johnson, Bayram Tali, Merijn Van De Klundert, Greg P Heath, E. 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Tabarelli de Fatis, Andrew Hart, Demetrios Loukas, Helio Nogima, Anastasia Karavdina, Suyong Choi, Etiennette Auffray, Maurizio Biasini, Daniele Trocino, Silvia Maselli, Rhys Taus, Sinan Sagir, Marta Felcini, Francesco Brivio, Marco Musich, Hannu Siikonen, Luis Junior Sanchez Rosas, Charalambos Nicolaou, Niki Saoulidou, Zhengcheng Tao, Jan Kieseler, Giulia Negro, Bożena Boimska, Antonio Delgado Peris, Frank Jensen, Sabino Meola, Roberto Covarelli, Sergio Cittolin, Jared Sturdy, Kaya Tatar, Elif Asli Yetkin, Sandra S. Padula, Kerem Cankocak, Thomas Weiler, Paolo Vitulo, Maximilian Knut Kiesel, William J Spalding, Konstantin Androsov, Tai Sakuma, Andrés Cabrera, Marc Stöver, Antonia Di Crescenzo, Anne-Marie Magnan, Wagner Carvalho, Deniz Sunar Cerci, Laszlo Gutay, Alberto Orso Maria Iorio, Harrison Prosper, Marta Baselga, Felice Pantaleo, Chanwook Hwang, Carley De Oliveira Martins, Stephen Robert Wagner, Kevin Deroover, Anterpreet Kaur, Niladribihari Sahoo, Sercan Sen, Winston Ko, Andre Govinda Stahl Leiton, Zhenyu Chen, Martina Malberti, Bhawandeep Bhawandeep, Kak Wong, Young Ho Shin, Yutaro Iiyama, Nikitas Loukas, Apichart Hortiangtham, Dezso Horvath, Mani Tripathi, Rachel Bartek, Reza Goldouzian, Mohd Nizam Yusli, Luisa Alunni Solestizi, Ryan Mueller, Marco Peruzzi, L. Lloret Iglesias, Usama Hussain, Owen Rosser Long, Warren Clarida, Intae Yu, Priyanka Priyanka, Sourav Dey, Jay Roberts, Stefano Bianco, Yury Ivanov, Andre Sznajder, Serdal Damarseckin, Illia Babounikau, Torben Dreyer, Alessia Tricomi, Krzysztof Nawrocki, Nikolay Tyurin, Jay Dittmann, Anna Elliott-Peisert, Vuko Brigljevic, Bruno Wittmer, Roumyana Hadjiiska, Terhi Jarvinen, Pallabi Das, Georg Steinbrück, Igor Smirnov, Daniel Tapia Takaki, Pawan Kumar Netrakanti, Alexander Dierlamm, Minna Leonora Vesterbacka Olsson, David Taylor, Renato Potenza, Aran Garcia-Bellido, Michal Szleper, Philippe Gras, Geoffrey Smith, Nicolas Postiau, Cesare Calabria, Franco Ligabue, Vytautas Dudenas, Kerstin Hoepfner, Eirini Tziaferi, Roberto Chierici, Chia-Ming Kuo, Guenter Eckerlin, Richard Loveless, Armen Tumasyan, Nicola Amapane, Malte Backhaus, Matteo Sani, Nicholas Wardle, Arka Santra, Andreas Nowack, Petar Adzic, Andrew Ackert, Yuri Gershtein, Emmanuelle Perez, Tao Huang, Cristina Riccardi, Daniele Vadruccio, Maria Margherita Obertino, Alajos Makovec, Francois Lagarde, Jack Wright, Candan Dozen, Michael Wayne Arenton, Kenneth Long, Andrea Carlo Marini, Alexander Tapper, Greg Landsberg, Cécile Caillol, Paula Eerola, Giuseppe Della Ricca, Sw. Banerjee, Manoj Sharan, Isa Dumanoglu, Vyacheslav Krutelyov, Barbara Clerbaux, Giacomo Sguazzoni, Alan Campbell, Muhammad Gul, Engin Eren, Colin Fallon, Vladimir Karjavine, Fatma Boran, Dalath Rachitha Mendis, Luisa Fernanda Chaparro Sierra, Deborah Pinna, Caterina Vernieri, Arnd Meyer, Alexis Fagot, Zhicai Zhang, Sean Kalafut, Shalini Thakur, James John Brooke, Cédric Prieels, Koushik Mandal, Paraskevas Sphicas, Michael Reichmann, Joscha Knolle, Anton Babaev, Marius Preuten, John N. Wood, Nils Faltermann, Manjit Kaur, Duong Nguyen, Michele Gallinaro, Elena Voevodina, Ioannis Papakrivopoulos, Praveen Chandra Tiwari, Martina Ressegotti, Rui Xiao, Evangelos Paradas, Kevin Burkett, Vladyslav Danilov, Marcello Maggi, Davide Piccolo, Vincenzo Monaco, Cristina Tuve, Humberto Antonio Salazar Ibarguen, Walter Van Doninck, Shawn Williamson, Fabrizio Gasparini, Michele Selvaggi, Richard Barbieri, Nabin Poudyal, Sharon Hagopian, Ralf Ulrich, Andreas Künsken, Pierre Van Mechelen, Junquan Tao, Alberto Benvenuti, Corrinne Mills, Maria Agnese Ciocci, Dave Pellett, Marko Kovac, Maria Florencia Canelli, Fabrizio Ferro, Thomas Ferbel, Dan Green, Giorgia Miniello, Peter Wittich, Laurent Thomas, Mark Derdzinski, Juliette Alimena, Gulsen Onengut, Viktor Matveev, Marta Ruspa, Zukhaimira Zolkapli, Krzysztof Piotrzkowski, Ekaterina Kuznetsova, Lloyd Stanley Durkin, Vincenzo Innocente, Clemens Lange, Francesco Fabozzi, Michal Olszewski, Chad Flores, Stefaan Tavernier, Ioannis Papadopoulos, Efstathios Paganis, Erica Brondolin, Santiago Folgueras, George Alverson, Roman Kogler, Miroslav Finger, Borislav Pavlov, Pablo Martinez Ruiz del Arbol, Csaba Hajdu, Emyr Clement, Nataliia Kovalchuk, Satoshi Hasegawa, Benjamin Kreis, Mark Pesaresi, Stepan Obraztsov, Anshul Kapoor, Fred-Markus Helmut Stober, Mario Masciovecchio, Claudia Ciocca, Dhanush Anil Hangal, Diego Ciangottini, David Petyt, Hans Rykaczewski, Chiara Mariotti, Geng Chen, Paul Schütze, Luca Brianza, Markus Seidel, Vineet Kumar, Giovanni Petrucciani, Victor Murzin, Yildiray Komurcu, Philippe Busson, Stefano Marcellini, Huilin Qu, James Letts, Vipin Bhatnagar, Houmani El Mamouni, Marco Monteno, Alexey Volkov, Alessio Boletti, Jie Zhang, Francesca Romana Cavallo, Giovanni Zevi Della Porta, Viktor Savrin, Mitchell Wayne, Karol Bunkowski, Miaoyuan Liu, Tutanon Sinthuprasith, Andrey Belyaev, Raffaella Radogna, Ece Aşılar, Sandeep Kaur, Tanvi Wamorkar, Lei Feng, Pedrame Bargassa, Katja Klein, Jens Multhaup, Giorgio Maggi, Sadia Khalil, Stefan Grünendahl, Amedeo Staiano, Robert Schöfbeck, Kamuran Dilsiz, Steven Wasserbaech, Seema Bahinipati, Paolo Rumerio, Lorenzo Uplegger, Jan Hoss, William T. Ford, Christian Autermann, Can You, Kenneth Bloom, Nick Amin, Philip Harris, Noemi Beni, Javier Fernandez Menendez, Nathaniel Woods, Maria Isabel Josa, Shashikant Dugad, Eva Halkiadakis, Raghav Kunnawalkam Elayavalli, Thomas Perry, Hannsjoerg Artur Weber, Gordon H. Hanson, Michel Della Negra, Nikolay Voytishin, Frank Glege, Iurii Antropov, Deborah Duchardt, Markus Radziej, Dylan Gilbert, Kira Burt, Sandhya Jain, Subir Sarkar, Seth Cooper, Semra Turkcapar, Viktor Kutzner, Philip Hebda, Linda Finco, Alfredo Castaneda Hernandez, Adriano Di Florio, Keith Rose, Mingshui Chen, Georgios Krintiras, Hannes Sakulin, Raffaele Gerosa, Huaqiao Zhang, Alexander Ledovskoy, Vincent J Smith, Yuri Andreev, Wenzhao Li, Jian-Guo Bian, Aysel Kayis Topaksu, Andrey Pozdnyakov, Thomas Kress, Tilman Rohe, Jing Wang, Matthias Komm, Arnab Purohit, Simona Cometti, Scott Thomas, Piero Giorgio Verdini, Matevz Tadel, Merve Nazlim Agaras, Mehar Ali Shah, Laura Dodd, Andrew Levin, Anton Stepennov, Andrey Gribushin, Predrag Cirkovic, Ashley Parker, Viola Sordini, Eduard De La Cruz-Burelo, Erika Garutti, Juan Manuel Grados Luyando, Ka Hei Martin Kwok, Filippo Errico, Deepak Kumar Sahoo, Jean-Louis Faure, Philipp Millet, Stefano Colafranceschi, Paolo Gunnellini, Gerrit Patrick Van Onsem, Ivan Heredia-De La Cruz, Brian Francis, Paolo Checchia, Giancarlo Mantovani, Carlo Battilana, Sezen Sekmen, Alberto Messineo, John Almond, Charles Ferraioli, Nicholas Eminizer, Pooja Saxena, Batool Safarzadeh, Daniele Ruini, Alice Magnani, Juliet Ritchie Patterson, Michail Bachtis, Duncan Carlsmith, Joao Varela, Bipen Singh, Leander Litov, Kyong Sei Lee, Jean-Pierre Merlo, Rocky Bala Garg, Maximilian Heindl, Claus Kleinwort, Alexander Savin, Caleb Fangmeier, Quentin Ingram, Igor Vorobiev, Joanne Cole, Eija Tuominen, Luigi Fiore, Martin Delcourt, Francesco Fallavollita, Julie Managan Hogan, Lucas Brito, Panos A Razis, Patrick Connor, Roberval Walsh, Giovanna Selvaggi, Steven R. Simon, John Gabriel Acosta, Laura Borrello, Daniel Abercrombie, Paul Lujan, Sifu Luo, Sergei Slabospitskii, Anne-Catherine Le Bihan, Gagan Bihari Mohanty, Gabor Istvan Veres, Sandeep Sharma, Alexandre Mertens, Nadja Strobbe, Jean-Laurent Agram, Anthony Moeller, Jim Freeman, Sarah Catherine Eno, Jan-Frederik Schulte, G. Bauer, Geum Bong Yu, Alberto Bragagnolo, Begona De La Cruz, Aristotelis Kyriakis, Cecilia Uribe Estrada, Ferenc Sikler, Dayong Wang, Mauro Verzetti, Isis Van Parijs, Antonio Vagnerini, Mario Kadastik, Francesca Cavallari, Stefano Belforte, Massimo Casarsa, Wanda Lucia Prado Da Silva, Rachel Yohay, F. Simonetto, Thomas Müller, Andrés G Delannoy, Christopher Hill, Pawel de Barbaro, Sergio P Ratti, Hugues Brun, Pieter Everaerts, Frank Chlebana, Titas Roy, Alexx Perloff, Roman Ryutin, Federica Primavera, Alexander Dermenev, Kuntal Mondal, Giovanni Organtini, Dong Ho Moon, Seyyed Mohammad Amin Ghiasi Shirazi, Adam Elwood, Nikolai Krasnikov, Sami Lehti, Adish Vartak, David Bertsche, Valentina Mariani, Alessia Saggio, Andreas Bernhard Meyer, Paolo Spagnolo, Ivan Shvetsov, Roberto Carlin, Igor Golutvin, Mircho Rodozov, Pierre Depasse, Vyacheslav Klyukhin, Stefan Michael Heindl, Maria Aldaya Martin, Jennifer Ngadiuba, Lindsey Gray, Nicola Bacchetta, Attila Racz, Roberta Arcidiacono, Christian Schnaible, Jonathan Fulcher, Anatoli Pashenkov, Avto Kharchilava, Mikhail Ignatenko, Jelena Luetic, Alberto Belloni, Tapio Lampén, Fabrizio Fabbri, Claudia Cecchi, Christoph Wissing, Norraphat Srimanobhas, Riccardo Di Maria, Dermot Moran, Jan Eysermans, Attilio Santocchia, Jean Fay, Igor Dremin, Abideh Jafari, Rogelio Reyes-Almanza, Nathan Mirman, Burak Bilki, Nicolò Trevisani, Dirk Krücker, Gianluca Cerminara, Lorenzo Russo, Jesus Manuel Vizan Garcia, Dustin Stolp, Lorenzo Viliani, Kurt Jung, Maria Savina, Anne-Laure Pequegnot, Gino Bolla, Adel Terkulov, Caglar Zorbilmez, Emrah Tiras, Toyoko Orimoto, Luciano Romero, Bolek Wyslouch, Maria Spiropulu, Christian Dorfer, D. M. Strom, Matthew Herndon, Thomas James, Alexey Kamenev, Sevgi Tekten, Fabio Cossutti, Mateusz Zarucki, Jovan Milosevic, Mareike Meyer, Dan Quach, Vitaliano Ciulli, Apostolos Panagiotou, Benjamin Kilminster, Hyun-Soo Kim, Christopher West, Si-Jin Qian, Isabel Ojalvo, Youn Roh, Barry Blumenfeld, Prasant Kumar Rout, Amitabh Lath, Simon Kudella, Riccardo Paramatti, Andrea Giammanco, Priyanka Kumari, Alberto Escalante Del Valle, Giorgio Apollinari, Ulf Behrens, W. A. T. Wan Abdullah, Jamal Rorie, Jason Gilmore, Marco Paganoni, Don Lincoln, Li Yuan, Jory Sonneveld, Hafeez R Hoorani, Rylan Conway, Daniel John Karmgard, Manfred Jeitler, Fabrizio Palla, Andrew Melo, Owen Baron, Mengyao Shi, Steve Schnetzer, Saranya Ghosh, Klaas Padeken, Renato Campanini, Gautier Hamel de Monchenault, Carlos Lourenco, Alexander Nehrkorn, Annapaola De Cosa, Drew Baden, Charles Mueller, Benjamin Mesic, Luca Perrozzi, Manfred Krammer, Kevin Sung, Florent Lacroix, Matthias Ulrich Mozer, Konstanty Sumorok, Semiray Girgis, George Wei-Shu Hou, Kyeongpil Lee, Teruki Kamon, Dmitry Elumakhov, James Buchanan, Maxim Pieters, Johannes Brandstetter, Ulrich Heintz, Arun Kumar, Helena Bialkowska, Alexander Malakhov, Efe Yazgan, Günter Flügge, Qiao Xu, Danyyl Brzhechko, Erhan Gülmez, Kaori Maeshima, Aurelijus Rinkevicius, Martin Erdmann, Andrew Wisecarver, Tyler Ruggles, Robert Clare, Sergey Petrushanko, Patricia McBride, Krzysztof Doroba, Pantelis Kontaxakis, Dylan Rankin, Andrew Brinkerhoff, Patrizia Azzi, Thomas Hebbeker, Paul Lecoq, Thomas Ferguson, Jose Flix, Ksenia Shchelina, Albert M. Sirunyan, Christian Scharf, Jangbae Lee, Didier Contardo, Chiara Amendola, Rostyslav Shevchenko, Sudeshna Banerjee, Vladimir Andreev, Ramandeep Kumar, Aruna Nayak, Michael Plagge, Gervasio Gomez, Frans Meijers, Edward Scott, Archana Sharma, Daniel Salerno, Rohan Bhandari, Vinay Hegde, Saptaparna Bhattacharya, David Zou, Andrey Korytov, P. Chang, Eduardo De Moraes Gregores, Ashfaq Ahmad, Vladimir Korenkov, Ashim Roy, Jung-Hyun Kim, Jan Krolikowski, Luiz Mundim, Duccio Abbaneo, Elizabeth Locci, Ilaria Vai, Gabriele Benelli, Patrizia Barria, Somnath Choudhury, Nazar Stefaniuk, Gregor Kasieczka, Oleksii Toldaiev, Adinda De Wit, Marco Meschini, Lesya Shchutska, Andrea Massironi, M. A. B. Ali, Markéta Jansová, Francesco Navarria, Juozas Vaitkus, Christopher George Tully, Alexander Belyaev, Claudio Campagnari, Teppo Mäenpää, Stephanie Brandt, Wolfgang Lohmann, Christopher Neu, Filip Moortgat, Soham Bhattacharya, Konstantinos Kousouris, Arne Reimers, Joshua Bendavid, Nicanor Colino, Alexis Pompili, Louie Corpe, Stephen Wimpenny, Henning Flacher, Nikolaos Manthos, Christian Laner, Martin Grunewald, Federico Preiato, Oleg Prokofyev, Wolfram Erdmann, Nicolo Cartiglia, Rajat Gupta, Mara Senghi Soares, Serguei Ganjour, Silvia Taroni, Juan Alcaraz Maestre, Raphael Granier de Cassagnac, Darien Wood, Jyothsna Rani Komaragiri, Satyaki Bhattacharya, Isabell-Alissandra Melzer-Pellmann, Nicholas John Hadley, Jehad Mousa, Karl Matthew Ecklund, Maral Alyari, Giuseppe Bagliesi, Sung Bin Oh, Jae Sung Kim, Songkyo Lee, Markus Stoye, Tatjana Susa, Vladimir Chekhovsky, Alain Hervé, Yuri Skovpen, Ivan Vila, William John Womersley, Peisen Ma, Suman Chatterjee, Tomas Lindén, Malte Hoffmann, Alice Florent, Carlo Civinini, Zhenan Liu, Andrea Triossi, Christoph Schwick, Richard Lander, Oh, Young, Do., Simone Gennai, Bibhuprasad Mahakud, G. Gomez Ceballos, Nikos Varelas, Ayse Bat, Helen F Heath, Kenichi Hatakeyama, Anna Woodard, Petr Levchenko, Marco Costa, Nikolai Golubev, Marcel Rieger, Anders Ryd, Gavin Davies, Sergey Vavilov, Alexander Lanev, Susan Dittmer, Kalyanmoy Chatterjee, Georgios Daskalakis, Mythra Varun Nemallapudi, Alessandra Romero, Sergei Gninenko, Petr Mandrik, Nicolas Filipovic, Senka Duric, Guler Karapinar, Sandro Fonseca De Souza, Muzamil Ahmad Bhat, Giuseppe Latino, Matthew Kilpatrick, Süleyman Durgut, John Paul Chou, Brian Paul Padley, Nairit Sur, Gregory Iles, Mohit Gola, and Jasper Lauwers

Subjects
Physics, Nuclear and High Energy Physics, Particle physics, Muon, Large Hadron Collider, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Supersymmetry, 01 natural sciences, Lightest Supersymmetric Particle, Massless particle, 0103 physical sciences, Transverse mass, ddc:530, High Energy Physics::Experiment, 010306 general physics, Lepton, Boson
Abstract

A search for direct production of the supersymmetric (SUSY) partners of electrons or muons is presented in final states with two opposite-charge, same-flavour leptons (electrons and muons), no jets, and large missing transverse momentum. The data sample corresponds to an integrated luminosity of 35.9fb$^{−1}$ of proton–proton collisions at s=13TeV, collected with the CMS detector at the LHC in 2016. The search uses the MT2 variable, which generalises the transverse mass for systems with two invisible objects and provides a discrimination against standard model backgrounds containing W bosons. The observed yields are consistent with the expectations from the standard model. The search is interpreted in the context of simplified SUSY models and probes slepton masses up to approximately 290, 400, and 450 GeV, assuming right-handed only, left-handed only, and both right- and left-handed sleptons (mass degenerate selectrons and smuons), and a massless lightest supersymmetric particle. Limits are also set on selectrons and smuons separately. These limits show an improvement on the existing limits of approximately 150 GeV.

Published
2019
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434. The PAU survey: Ly$\alpha$ intensity mapping forecast

Author

Pablo Renard, Laura Cabayol, J. Carretero, Juan Garcia-Bellido, Enrique Gaztanaga, Martin Eriksen, Ramon Miquel, Enrique Fernández, P. Tallada-Crespí, C. Padilla, Rupert A. C. Croft, E. J. Sanchez, UAM. Departamento de Física Teórica, Ministerio de Economía y Competitividad (España), Ministerio de Ciencia e Innovación (España), European Commission, Generalitat de Catalunya, Durham University, ETH Zurich, Leiden University, Netherlands Organization for Scientific Research, Universidad Autónoma de Barcelona, and National Aeronautics and Space Administration (US)

Subjects
Physics, Large-Scale Structure of Universe, Large-scale structure of Universe, Horizon (archaeology), 010308 nuclear & particles physics, Cosmology: observations, Física, Library science, Astronomy and Astrophysics, 01 natural sciences, Port (computer networking), Observations [Cosmology], Scale Structure of Universe, Space and Planetary Science, 0103 physical sciences, Large, media_common.cataloged_instance, European union, 010303 astronomy & astrophysics, media_common, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

In thiswork,we explore the application of intensity mapping to detect extended Ly α emission from the IGM via cross-correlation of PAUS images with Ly α forest data from eBOSS and DESI. Seven narrow-band (FWHM = 13 nm) PAUS filters have been considered, ranging from 455 to 515 nm in steps of 10 nm, which allows the observation of Ly α emission in a range 2.7 < z< 3.3. The cross-correlation is simulated first in an area of 100 deg2 (PAUS projected coverage), and second in two hypothetical scenarios: A deeper PAUS (complete up to iAB < 24 instead of iAB < 23, observation time ×6), and an extended PAUS coverage of 225 deg2 (observation time ×2.25). A hydrodynamic simulation of size 400 Mpc h-1 is used to simulate both extended Ly α emission and absorption, while the foregrounds in PAUS images have been simulated using a lightcone mock catalogue. Using an optimistic estimation of uncorrelated PAUS noise, the total probability of a non-spurious detection is estimated to be 1.8 per cent and 4.5 per cent for PAUS-eBOSS and PAUS-DESI, from a run of 1000 simulated cross-correlations with different realisations of instrumental noise and quasar positions. The hypothetical PAUS scenarios increase this probability to 15.3 per cent (deeper PAUS) and 9.0 per cent (extended PAUS). With realistic correlated noise directly measured from PAUS images, these probabilities become negligible. Despite these negative results, some evidences suggest that this methodology may be more suitable to broad-band surveys., The PAU Survey is partially supported by MINECO under grants CSD2007-00060, AYA2015-71825, ESP2017-89838, PGC2018-094773, PGC2018-102021, SEV-2016-0588, SEV-2016-0597, MDM-2015-0509, and Juan de la Cierva fellowship and LACEGAL and EWC Marie Sklodowska-Curie grants 734374 and 776247 with ERDF funds from the EU Horizon 2020 Programme, some of which include ERDF funds from the European Union. IEEC and IFAE are partially funded by the CERCA and Beatriu de Pinos programme of the Generalitat de Catalunya. Funding for PAUS has also been provided by Durham University (via the ERC StG DEGAS-259586), ETH Zurich, Leiden University [via ERC StG ADULT-279396, and Netherlands Organisation for Scientific Research (NWO) Vici grant no. 639.043.512], University College London and from the European Union’s Horizon 2020 research and innovation programme under the grant agreement no. 776247 EWC. The PAU data centre is hosted by the Port d’Informació Científica (PIC), maintained through a collaboration of CIEMAT and IFAE, with additional support from Universitat Autònoma de Barcelona and ERDF. We acknowledge the PIC services department team for their support and fruitful discussions. RACC was supported by NASA NNX17AK56G, NASA ATP-80NSSC18K101, NSF AST-1614853, and NSF AST-1615940.

Published
2020

435. The mystery of photometric twins DES17X1boj and DES16E2bjy

Author

A. Roodman, Daniel Scolnic, Peter Nugent, C. B. D'Andrea, Elisabeth Krause, Edward Macaulay, A. G. Kim, L. Kelsey, Juan Garcia-Bellido, A. Carnero Rosell, Ramon Miquel, P. Doel, D. L. Burke, J. Gschwend, Josh Frieman, R. L. C. Ogando, Lluís Galbany, W. C. Wester, D. J. Brout, Enrique Gaztanaga, Mathew Smith, Samuel Hinton, Mark Sullivan, N. Castro Segura, A. A. Plazas, F. Paz-Chinchón, Michael Schubnell, G. Gutierrez, T. F. Eifler, M. Childress, T. Muller, C. Angus, C. Lidman, B. E. Tucker, M. E. C. Swanson, E. Swann, M. March, P. Wiseman, N. E. Sommer, E. Suchyta, David J. James, Bruce A. Bassett, B. Flaugher, E. Buckley-Geer, Daniel Gruen, Claudia P. Gutiérrez, Felipe Menanteau, D. W. Gerdes, Tamara M. Davis, Gregory Tarle, M. Vincenzi, H. T. Diehl, M. A. G. Maia, B. P. Thomas, S. Everett, K. Honscheid, M. Carrasco Kind, J. De Vicente, Cosimo Inserra, Anais Möller, E. Bertin, D. L. Hollowood, I. Sevilla-Noarbe, S. Serrano, Richard Kessler, David Brooks, L. N. da Costa, Ryan J. Foley, M. Pursiainen, S. Allam, Robert A. Gruendl, Daniela Carollo, M. Grayling, Santiago Avila, S. Desai, Kyler Kuehn, Geraint F. Lewis, T. M. C. Abbott, C. Frohmaier, E. J. Sanchez, J. Annis, Jennifer L. Marshall, Antonella Palmese, V. Scarpine, Laboratoire de Physique de Clermont (LPC), Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), 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, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne (UCA)-Centre National de la Recherche Scientifique (CNRS), Dark Energy Survey, Science and Technology Facilities Council (UK), European Commission, European Research Council, Ministerio de Economía y Competitividad (España), Generalitat de Catalunya, and Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Clermont Auvergne [2017-2020] (UCA [2017-2020])-Centre National de la Recherche Scientifique (CNRS)

Subjects
Software_OPERATINGSYSTEMS, ComputingMethodologies_SIMULATIONANDMODELING, FOS: Physical sciences, Astrophysics, Data_CODINGANDINFORMATIONTHEORY, Astronomy & Astrophysics, 01 natural sciences, supernovae: general, 0103 physical sciences, medicine, Hardware_INTEGRATEDCIRCUITS, Black-body radiation, Absorption (electromagnetic radiation), 010303 astronomy & astrophysics, STFC, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, astro-ph.HE, Spiral galaxy, 010308 nuclear & particles physics, RCUK, Astronomy and Astrophysics, ComputerSystemsOrganization_PROCESSORARCHITECTURES, Light curve, Galaxy, ST/R000506/1, Supernova, medicine.anatomical_structure, Space and Planetary Science, Dark energy, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Nucleus, general [supernovae], Astronomical and Space Sciences
Abstract

DES Collaboration: et al., We present an analysis of DES17X1boj and DES16E2bjy, two peculiar transients discovered by the Dark Energy Survey (DES). They exhibit nearly identical double-peaked light curves that reach very different maximum luminosities (Mr = −15.4 and −17.9, respectively). The light-curve evolution of these events is highly atypical and has not been reported before. The transients are found in different host environments: DES17X1boj was found near the nucleus of a spiral galaxy, while DES16E2bjy is located in the outskirts of a passive red galaxy. Early photometric data are well fitted with a blackbody and the resulting moderate photospheric expansion velocities (1800 km s−1 for DES17X1boj and 4800 km s−1 for DES16E2bjy) suggest an explosive or eruptive origin. Additionally, a feature identified as high-velocity Ca II absorption (⁠v ≈ 9400 km s−1) in the near-peak spectrum of DES17X1boj may imply that it is a supernova. While similar light-curve evolution suggests a similar physical origin for these two transients, we are not able to identify or characterize the progenitors., We acknowledge support from the European Union’s 7th Framework Programme (EU/FP7) European Research council (ERC) grant 615929, and Science and Technology Facilities Council (STFC) grant ST/R000506/1. LG was funded by the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 839090. 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 MINECO under grants AYA2015-71825, ESP2015-66861, FPA2015-68048, SEV-2016-0588, SEV2016-0597, 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 Programme (FP7/2007-2013) including ERC grant agreements 240672, 291329, and 306478. We acknowledge support from the Brazilian Instituto Nacional de Ciencia e Tecnologia (INCT) e-Universe (CNPq grant 465376/2014-2).

Published
2020
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436. Non-Gaussian elliptic-flow fluctuations in PbPb collisions at sNN=5.02TeV

Author

Colin Bernet, Nadia Pastrone, Ugur Kiminsu, Martti Raidal, Pamela Klabbers, Francesca Cavallari, Pushpalatha C Bhat, Burin Asavapibhop, Aram Avetisyan, Amparo Lopez Virto, Matthew Nguyen, Pedro G Mercadante, Stefano Belforte, Massimo Casarsa, Thomas Müller, Andrés G Delannoy, Christopher Hill, Pawel de Barbaro, Alexandre Zabi, Vladimir Rekovic, Igor Miagkov, Bo Liu, Hans-Christian Kaestli, Zhangqier Wang, Mia Tosi, Marino Missiroli, Andrius Juodagalvis, Souvik Das, Alexander Dermenev, Andrey Popov, Dong Ho Moon, Agostino Di Francesco, Seyyed Mohammad Amin Ghiasi Shirazi, Adam Elwood, Nikolai Krasnikov, Lawrence Sulak, Pierluigi Paolucci, Vladimir Karjavin, Kerstin Borras, Sami Lehti, Adish Vartak, Valentina Mariani, Prashant Shukla, Zuhal Seyma Demiroglu, Daniel Meister, Thomas Strebler, André Rosowsky, Andrew Ivanov, Ivan Shvetsov, Igor Golutvin, Mircho Rodozov, Dong-Chul Son, Liliana Teodorescu, David Curry, Adolf Bornheim, Maria Aldaya Martin, Jennifer Ngadiuba, Aaron Bundock, Katerina Lipka, Marc Osherson, Matteo Centis Vignali, Martin Kirakosyan, Ruslan Chistov, Kadri Ozdemir, Tirso Alejandro Gómez Espinosa, Nicola Bacchetta, Attila Racz, Roberta Arcidiacono, Christian Schnaible, Jonathan Fulcher, Anatoli Pashenkov, Mikhail Ignatenko, Jelena Luetic, Tapio Lampén, Adrian Perieanu, Fabrizio Fabbri, Claudia Cecchi, Roy Montalvo, Dominic Smith, Howard Wells Wulsin, Clément Leloup, Reddy Pratap Gandrajula, Alexander Nikitenko, Jasvinder A. Singh, Christoph Wissing, Heriberto Castilla-Valdez, Adam Dishaw, Claudia Seitz, Alessandro Degano, Rishika Bhardwaj, János Karancsi, Norraphat Srimanobhas, Cécile Caillol, Riccardo Di Maria, Dermot Moran, Christopher Mcginn, David Yu, Daniel Robert Marlow, Thea Klaeboe Aarrestad, Haiyan Wang, Stefano Colafranceschi, Quan Wang, Yves Sirois, Mehmet Oglakci, Robert Hirosky, Sarah Freed, Zhixing Wang, Dipanwita Dutta, Jing Li, Alexei Safonov, Janos Erö, José Cupertino Ruiz Vargas, Sudha Ahuja, Halil Saka, Pietro Govoni, Monica Vazquez Acosta, Andrzej Pyskir, Alicia Calderon, Karl Gill, Sachiko Toda, Seyed Mohsen Etesami, Sandra Oliveros, Alfredo Gurrola, Samuel Bein, Ufuk Guney Tok, Shawn Zaleski, Cecilia Elena Gerber, Diego Beghin, Gian Michele Innocenti, Livia Soffi, Christopher Seez, Jian Wang, Ada Solano, Christopher Brew, Caleb Fangmeier, Lothar At Bauerdick, Leonardo Giannini, Quentin Ingram, Igor Vorobiev, Paolo Gunnellini, Francesca Romana Cavallo, Batool Safarzadeh, Felice Pantaleo, Juliet Ritchie Patterson, Vyacheslav Valuev, Joao Varela, Joachim Mnich, Nabin Poudyal, Andreas Mussgiller, Andreas Psallidas, Martin Delcourt, Douglas Wright, Giacomo Fedi, Francesco Fallavollita, Ivan-Kresimir Furic, Rishi Patel, Juan Pablo Fernández Ramos, Elias Pree, Virgil E. Barnes, Mihee Jo, Yacine Haddad, S. Sanchez Cruz, Mauro Menichelli, Luca Perniè, Roland Horisberger, Yuan Chao, Georgios Mavromanolakis, Michele Arneodo, Michele Gulmini, Eric Wayne Vaandering, Navid Rad, Yagya Raj Joshi, Fotios Ptochos, Andrea Perrotta, Fuqiang Wang, Kamuran Dilsiz, Iasonas Topsis-Giotis, Alexander Toropin, Jesus Puerta Pelayo, Gaetano-Marco Dallavalle, Samuel Higginbotham, Leander Litov, Kyong Sei Lee, Salvatore Costa, Indara Suarez, Yong Ban, Michele De Gruttola, Julie Managan Hogan, Sridhara Dasu, Lucas Brito, Steven R. Simon, Ajeeta Khatiwada, John Gabriel Acosta, Laura Borrello, Paul Lujan, Serhat Atay, Elisa Manoni, Alice Cocoros, Rocky Bala Garg, Joanne Cole, Mate Csanad, Sergey Polikarpov, Justin Pilot, Dominick Olivito, Panagiotis Katsoulis, Colin Jessop, Manuel Olmedo Negrete, Maciej Misiura, Hongfang Liu, Anna Teresa Meneguzzo, David Ja Cockerill, Wolfgang Lange, Gianni Masetti, Erik Gottschalk, Andrea Delgado, Joern Schwandt, Yen-Jie Lee, Pablo De Castro Manzano, Metin Yalvac, Stephan Lammel, Tagir Aushev, Riccardo Bellan, Torben Dreyer, Duncan Leggat, Yuriy Pakhotin, Shilpi Jain, Doga Gulhan, Louis Lyons, Jaana Kristiina Heikkilä, Christopher Anelli, Brieuc Francois, Brian L Winer, Mehmet Özgür Sahin, Donato Creanza, Marc Dobson, Heiner Tholen, Maryam Zeinali, Patrick Jarry, Benjamin Charles Radburn-Smith, Kevin Nash, Paul Edmund Karchin, Thomas Madlener, Daniel Pitzl, Akram Khan, Susan Gascon, Gunther Roland, Eija Tuominen, Valentina Dutta, Yue Shi Lai, Lucia Perrini, Alessio Ghezzi, Patrick Connor, Roberval Walsh, Wolfgang Funk, Illia Khvastunov, Suresh C Tonwar, Hugo Delannoy, Daniel Noonan, Sylvie Braibant-Giacomelli, Philipp Pigard, Jeffrey Roskes, Javier Andres Brochero Cifuentes, Anne-Catherine Le Bihan, Thomas Bergauer, Michael Planer, James Alexander, Lukasz Kreczko, Alessio Magitteri, Christian Schomakers, Johannes Grossmann, Vadim Oreshkin, Vladimir Mossolov, Ridhi Chawla, Byung-Sik Hong, Stefano Casasso, I. 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N. Butler, Fabiola Vazquez Valencia, Genius Walia, Dmitry Sosnov, Rudolf Fruehwirth, Nick Van Remortel, Chad Freer, Stefan Piperov, Daniel Arcaro, Constantin Heidegger, David Jonathan Hofman, Leonid Levchuk, Luca Scodellaro, Christos Roskas, Maria Cepeda, Giles Strong, Jorgen D'Hondt, Bahareh Roozbahani, Marek Walczak, Christine Mclean, Kunal Kothekar, Marcella Diemoz, Vladimir Epshteyn, Matti J Kortelainen, Natale Demaria, Daniele Marconi, Nazar Bartosik, Enrique Palencia Cortezon, Vladimir Popov, Otman Charaf, Simon Knutzen, Jacopo Pazzini, Silvio Donato, Ezio Torassa, Shubham Pandey, Wei Shi, Andrea Castro, Luis Junior Sanchez Rosas, Thomas Klijnsma, Stanislav Lisniak, Konstantin Androsov, Shirin Chenarani, Jozsef Molnar, Valerio Re, Harry Cheung, Andrew Johnson, Jordan Nash, Giuseppe Fasanella, Sung Keun Park, Zhen Hu, Keith Ulmer, Tai Sakuma, Zoltan Laszlo Trocsanyi, J. Conway, D. Del Re, Kevin Deroover, Andrew Melo, Bugra Bilin, Cheng-Chieh Peng, Kati Lassila-Perini, Gregory R. Snow, Seth Cooper, James G Branson, Juska Pekkanen, Helio Nogima, Robert Harr, Semra Turkcapar, Linda Finco, Alfredo Castaneda Hernandez, Anastasia Karavdina, Mohsen Naseri, Victor Murzin, Keith Rose, Mingshui Chen, Olivér Surányi, Charles Maguire, Alexander Grohsjean, Yueh-Feng Liu, Dimitrios Tsitsonis, Peter Thomassen, Adrián Quintario Olmeda, Phillip Russell Dudero, Lev Uvarov, Rajdeep Mohan Chatterjee, Stilianos Kesisoglou, Giorgia Rauco, Nancy Marinelli, Nicola Pozzobon, Dmitry Shtol, Petra Van Mulders, Bajrang Sutar, Elizabeth Starling, René Caspart, Rajarshi Bhattacharya, Elisabetta Manca, Gérald Grenier, Christoph Grab, Nadeesha Wickramage, Anna Zanetti, Tobias Pook, Jay Hauser, Alessandro Braghieri, Johannes Schulz, Mustafa Numan Bakirci, Dustin Stolp, Lorenzo Viliani, David Sperka, Gaelle Boudoul, Dong Hee Kim, Kurt Jung, Geng-Yuan Jeng, Irene Bachiller, Cristina Biino, Ivan Mikulec, Francesco Micheli, Gul Gokbulut, Alexis Kalogeropoulos, Savvas Kyriacou, Denis Rathjens, Alexander Schmidt, Vincent Lemaitre, Gianni Zumerle, Klaas Padeken, Mark Foerster, Sunil Bansal, Stefano Lacaprara, Nicholas Smith, Emanuele Di Marco, Henning Kirschenmann, Edouard Boos, Miaoyuan Liu, Jesus Marco, Sebastian Baur, David Krofcheck, Elif Asli Yetkin, Alberto Orso Maria Iorio, Chanwook Hwang, Andrei Starodumov, Isidro Gonzalez Caballero, Florian Kassel, Michael Brodski, Niladribihari Sahoo, Apichart Hortiangtham, Dezso Horvath, Tutanon Sinthuprasith, Jonathan Hollar, Willis Lin, Florian Zenoni, John Strologas, Theodoros Geralis, Andrea Rizzi, Clemens Wöhrmann, Svenja Schumann, Jean-Charles Fontaine, Tielige Mengke, Salvatore Buontempo, Paul Avery, Salavat Abdullin, Lisa Benato, Manuel Alejandro Segura Delgado, Isabelle De Bruyn, Quentin Python, Katja Klein, Randy Ruchti, Joe Incandela, Luca Cadamuro, Virginia Azzolini, Gobinda Majumder, Manuel Franco Sevilla, Marvin Johnson, Dooyeon Gyun, Alexey Volkov, Yutaro Iiyama, Intae Yu, Gregory Rakness, Giacomo Bruno, Manuel Calderon De La Barca Sanchez, Tomas Hreus, Damir Devetak, Anna Elliott-Peisert, Michele Bianco, Vuko Brigljevic, Roger Rusack, Marc Dejardin, Olena Karacheban, Petra Merkel, De Hua Zhu, Marco De Mattia, Jorge Chaves, Paul Baillon, Cristóvão Beirão Da Cruz E Silva, Artur Apresyan, Marc Besancon, Dinyar Rabady, Lucia Silvestris, David Taylor, Wolfram Dietrich Zeuner, Bora Akgun, Aran Garcia-Bellido, Si Xie, Luigi Benussi, Robert Stone, Gouranga Kole, Bruno Galinhas, Irving Daniel Sandoval Gonzalez, Nicolas Zaganidis, Silvia Goy Lopez, Zoltan Gecse, Jongseok Lee, Luigi Fiore, Wenzhao Li, Matthias Komm, Arnab Purohit, Scott Thomas, Piero Giorgio Verdini, Matevz Tadel, Plamen Iaydjiev, Yang Yang, Luigi Guiducci, Jared Turkewitz, Nathaniel Woods, Luisa Alunni Solestizi, Ryan Mueller, Anirban Saha, Andrew Evans, Kenyi Hurtado Anampa, Guenakh Mitselmakher, Jordan Damgov, D. 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Zhemchugov, Eduardo Coelho, Roumyana Hadjiiska, Igor Smirnov, Andreas Hinzmann, Marco Verzocchi, Ozlem Kaya, Sam Harper, Vytautas Dudenas, Yeonju Go, Nikolay Terentyev, Christophe Ochando, Kerstin Hoepfner, Sevil Salur, Francesco Santanastasio, Stoyan Stoynev, Morgan Lethuillier, Yasar Onel, Jonatan Piedra Gomez, Fanbo Meng, Jhovanny Mejia Guisao, Caroline Collard, Johannes Hauk, Antonio María Pérez-Calero Yzquierdo, Kenneth Long, Andrea Carlo Marini, Alexander Tapper, Vyacheslav Krutelyov, Matthew Jones, Luisa Fernanda Chaparro Sierra, Deborah Pinna, Caterina Vernieri, Juan Garcia-Ferrero, Alexei Raspereza, Supratik Mukhopadhyay, Georgios Anagnostou, Melody A. Swartz, Maxwell Chertok, Mauro De Palma, Naimuddin, Ravi Janjam, Siddharth Narayanan, Anton Karneyeu, Leonard Apanasevich, Weinan Si, Menglei Sun, Jeremy Mans, Peter Schleper, Salvatore Nuzzo, Markus Radziej, Jochen Schieck, Giancarlo Mantovani, Carlo Battilana, Sezen Sekmen, Charles Ferraioli, Pooja Saxena, Dylan Gilbert, Gian Mario Bilei, Philippe Bloch, Gyorgy Bencze, Dimitri Bourilkov, Andrew Whitbeck, Grant Riley, Robert Fischer, Richard Loveless, Viktor Veszpremi, Abdulla Abdulsalam, Charalambos Nicolaou, Niki Saoulidou, Zhengcheng Tao, Philip Hebda, Hannu Siikonen, Frank Jensen, Martina Malberti, Ignacio Redondo, Benjamin Stieger, Hyun-Chul Kim, Yurii Maravin, Vladimir Gavrilov, Shuichi Kunori, Asif Saddique, Stephane Perries, Carsten Heidemann, Costas Foudas, Rebeca Gonzalez Suarez, Devdatta Majumder, Jay Dittmann, Daniel Tapia Takaki, Pawan Kumar Netrakanti, Alessandro Rossi, Matthias Schröder, Xavier Coubez, Fabrice Couderc, Alex Garabedian, Egidio Longo, Francesca Ricci-Tam, Federico De Guio, Ivan Marchesini, Mohsan Waseem Ather, Anna Stakia, Sébastien Wertz, Vishwajeet Jha, Salvatore Rappoccio, Petar Adzic, Paolo Azzurri, Rylan Conway, Ferdos Rezaei Hosseinabadi, Günther Dissertori, Yi Chen, Jay Mathew Lawhorn, Claude Amsler, Brent Yates, Zhoudunming Tu, Danek Kotlinski, Simone Gelli, Ian Macneill, Tongguang Cheng, Sergo Jindariani, Caleb Smith, John Bradmiller-Feld, Rino Castaldi, John Hakala, Alexander Bylinkin, Daniel Teyssier, John Yelton, Anterpreet Kaur, Hongbo Liao, Rainer Mankel, Mariana Shopova, Eric Christian Chabert, Aleko Khukhunaishvili, Sean Flowers, Sandeep Bhowmik, Thiago Tomei, Sonaina Undleeb, Elizaveta Nazarova, Julie Malcles, Fengwangdong Zhang, Victor Perelygin, Alessandra Fanfani, Yi-ting Duh, Boris Grynyov, Denis Gelé, Chang-Seong Moon, Mauro Emanuele Dinardo, Carmen Albajar, Sven Dildick, Jingzhou Zhao, Abhigyan Dasgupta, Zviad Tsamalaidze, Nikolai Skatchkov, Louis Antonelli, Nhan Viet Tran, Mohammad Abrar Wadud, Markus Friedl, Marek Niedziela, Laurent Favart, Kristof Pauwels, Cristian Pena, Thomas Reis, K. 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Subjects
Physics, Nuclear and High Energy Physics, Particle physics, 010308 nuclear & particles physics, Gaussian, Elliptic flow, 01 natural sciences, Charged particle, Nuclear physics, symbols.namesake, Skewness, Pseudorapidity, Non-Gaussianity, 0103 physical sciences, Quark–gluon plasma, symbols, High Energy Physics::Experiment, Rapidity, Nuclear Experiment, 010306 general physics
Abstract

Event-by-event fluctuations in the elliptic-flow coefficient v2 are studied in PbPb collisions at sNN=5.02 TeV using the CMS detector at the CERN LHC. Elliptic-flow probability distributions p(v2) for charged particles with transverse momentum 0.3

Published
2019
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437. The Diffuse Light Envelope of Luminous Red Galaxies

Author

Yanxi Zhang, Eli S. Rykoff, G. Gutierrez, Antonella Palmese, M. A. G. Maia, M. E. C. Swanson, B. Flaugher, J. Carretero, A. Carnero Rosell, Juan Garcia-Bellido, E. Bertin, Kyler Kuehn, M. Costanzi, Brian Yanny, A. K. Romer, K. Herner, J. Annis, A. Roodman, I. Sevilla-Noarbe, David J. James, N. Kuropatkin, T. N. Varga, L. N. da Costa, Sunayana Bhargava, K. Honscheid, Marcos Lima, Michael Schubnell, H. Sampaio-Santos, S. Everett, V. Scarpine, R. L. C. Ogando, V. Strazzullo, S. Serrano, Ramon Miquel, J. Gschwend, A. A. Plazas, Josh Frieman, E. Suchyta, D. L. Burke, Peter Doel, S. Allam, Robert A. Gruendl, H. T. Diehl, David J. Brooks, M. Carrasco Kind, Michel Aguena, T. F. Eifler, Enrique Gaztanaga, E. J. Sanchez, Santiago Avila, Y. Leung, S. Desai, F. Paz-Chinchón, M. Smith, Daniel Gruen, A. G. Kim, 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, Leung, Y., Zhang, Y., Yanny, B., Herner, K., Annis, J., Palmese, A., Sampaio-Santos, H., Strazzullo, V., Aguena, M., Allam, S., Avila, S., Bertin, E., Bhargava, S., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Costanzi, M., da Costa, L. N., Desai, S., Diehl, H. T., Doel, P., Eifler, T. F., Everett, S., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Honscheid, K., James, D. J., Kim, A. G., Kuehn, K., Kuropatkin, N., Lima, M., Maia, M. A. G., Miquel, R., Ogando, R. L. C., Paz-Chinchón, F., Plazas, A. A., Romer, A. K., Roodman, A., Rykoff, E. S., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Swanson, M. E. C., and Varga, T. N.

Subjects
Physics, 010308 nuclear & particles physics, FOS: Physical sciences, Flux, General Medicine, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Astrophysics - Astrophysics of Galaxies, Galaxy, Redshift, Astrophysics of Galaxies (astro-ph.GA), Galaxy evolution, 0103 physical sciences, Galaxy formation and evolution, Diffuse reflection, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], 010303 astronomy & astrophysics, Sersic profile, Astrophysics::Galaxy Astrophysics, Envelope (waves)
Abstract

We use a stacking method to study the radial light profiles of luminous red galaxies (LRGs) at redshift ∼0.62 and ∼0.25, out to a radial range of 200 kpc. We do not find noticeable evolution of the profiles at the two redshifts. The LRG profiles appear to be well approximated by a single Sérsic profile, although some excess light can be seen outside 60 kpc. We quantify the excess light by measuring the integrated flux and find that the excess is about 10%—a non-dominant but still nonnegligible component.

Published
2020
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438. The STRong lensing Insights into the Dark Energy Survey (STRIDES) 2017/2018 follow-up campaign: discovery of 10 lensed quasars and 10 quasar pairs

Author

A. A. Plazas, C. Lemon, Antonella Palmese, M. Smith, M. A. G. Maia, G C-F Chen, J. Carretero, Anowar J. Shajib, Marcos Lima, Adriano Agnello, Frederic Courbin, Ramon Miquel, Shantanu Desai, D. L. Burke, G. Gutierrez, G. Tarle, Daniel Gruen, M. March, Ofer Lahav, Paul L. Schechter, Tim Eifler, Enrique Gaztanaga, Thomas E. Collett, A. Carnero Rosell, M. Costanzi, Yordanka Apostolovski, Kyler Kuehn, Juan Garcia-Bellido, Richard G. McMahon, Christopher D. Fassnacht, S. Allam, Robert A. Gruendl, Elisabeth Krause, David J. Brooks, A. Melo, Simon Birrer, Motta, David J. James, D. W. Gerdes, Matthew W. Auger, Michael Schubnell, Tommaso Treu, Josh Frieman, Cristian E. Rusu, Felipe Menanteau, M. Carrasco Kind, A. Roodman, B. Flaugher, J. Annis, Alistair R. Walker, Marcelle Soares-Santos, Timo Anguita, E. Suchyta, S. Serrano, K. Honscheid, N. Kuropatkin, F. Paz-Chinchón, Santiago Avila, Jennifer L. Marshall, L. N. da Costa, A. G. Kim, J. De Vicente, Huan Lin, E. Buckley-Geer, T. M. C. Abbott, E. Bertin, E. J. Sanchez, J. Gschwend, Lemon, C., Auger, M. W., Mcmahon, R., Anguita, T., Apostolovski, Y., Chen, G. C. -F., Fassnacht, C. D., Melo, A. D., Motta, V., Shajib, A., Treu, T., Agnello, A., Buckley-Geer, E., Schechter, P. L., Birrer, S., Collett, T., Courbin, F., Rusu, C. E., Abbott, T. M. C., Allam, S., Annis, J., Avila, S., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Eifler, T. F., Flaugher, B., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Honscheid, K., James, D. J., Kim, A., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Lin, H., Maia, M. A. G., March, M., Marshall, J. L., Menanteau, F., Miquel, R., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Roodman, A., Sanchez, E., Schubnell, M., Serrano, S., Smith, M., Soares-Santos, M., Suchyta, E., Tarle, G., Walker, A. R., 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, McMahon, Richard [0000-0001-8447-8869], and Apollo - University of Cambridge Repository

Subjects
candidates, observational [methods], time-delay, Astrophysics, 01 natural sciences, Astrophysics::Solar and Stellar Astrophysics, 010303 astronomy & astrophysics, sky, Physics, Faint Object Spectrograph, Astrophysics::Instrumentation and Methods for Astrophysics, gravitational lensing: strong, gravitational lenses, strong [gravitational lensing], Astrophysics::Earth and Planetary Astrophysics, methods: observational, sextractor, Astronomical and Space Sciences, astro-ph.GA, FOS: Physical sciences, selection, Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy & Astrophysics, Photometry (optics), quasars: general, Gravitational Lenses, 0103 physical sciences, Quasars, Spectrograph, STFC, Astrophysics::Galaxy Astrophysics, general [quasars], 010308 nuclear & particles physics, variability, Near-infrared spectroscopy, RCUK, Astronomy and Astrophysics, Quasar, Galaxies, Light curve, redshift, Astrophysics - Astrophysics of Galaxies, Redshift, Galaxy, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), gaia, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], cosmograil
Abstract

We report the results of the STRong lensing Insights from the Dark Energy Survey (STRIDES) follow-up campaign of the late 2017/early 2018 season. We obtained spectra of 65 lensed quasar candidates either with EFOSC2 on the NTT or ESI on Keck, which confirm 10 new gravitationally lensed quasars and 10 quasar pairs with similar spectra, but which do not show a lensing galaxy in DES images. Eight lensed quasars are doubly imaged with source redshifts between 0.99 and 2.90, one is triply imaged by a group (DESJ0345-2545, $z=1.68$), and one is quadruply imaged (quad: DESJ0053-2012, $z=3.8$). Singular isothermal ellipsoid models for the doubles, based on high-resolution imaging from SAMI on SOAR or NIRC2 on Keck, give total magnifications between 3.2 and 5.6, and Einstein radii between 0.49 and 1.97 arcseconds. After spectroscopic follow-up, we extract multi-epoch $grizY$ photometry of confirmed lensed quasars and contaminant quasar+star pairs from the first 4 years of DES data using parametric multi-band modelling, and compare variability in each system's components. By measuring the reduced ${\chi}^2$ associated with fitting all epochs to the same magnitude, we find a simple cut on the less variable component that retains all confirmed lensed quasars, while removing 94 per cent of contaminant systems with stellar components. Based on our spectroscopic follow-up, this variability information can improve selection of lensed quasars and quasar pairs from 34-45 per cent to 51-70 per cent, with the majority of remaining contaminants being compact star-forming galaxies. Using mock lensed quasar lightcurves we demonstrate that selection based only on variability will over-represent the quad fraction by 10 per cent over a complete DES magnitude-limited sample (excluding microlensing differences), explained by the magnification bias and hence lower luminosity (more variable) sources in quads., Comment: 22 pages, 16 figures, submitted to MNRAS

Published
2020
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439. Blinding multiprobe cosmological experiments

Author

Michael Troxel, Matt J. Jarvis, Kyler Kuehn, I. Sevilla-Noarbe, Tim Eifler, Josh Frieman, N. Kuropatkin, G. Tarle, Jochen Weller, Shantanu Desai, J. Gschwend, Alistair R. Walker, Gary Bernstein, W. G. Hartley, L. N. da Costa, M. Smith, Ramon Miquel, W. C. Wester, Peter Melchior, Daniel Gruen, E. J. Sanchez, Michael Schubnell, David J. James, A. A. Plazas, Felipe Menanteau, Elisabeth Krause, Pablo Fosalba, R. Cawthon, Antonella Palmese, Keith Bechtol, E. Bertin, D. L. Burke, J. Carretero, Santiago Avila, Daniel Thomas, D. W. Gerdes, E. Buckley-Geer, F. Elsner, Peter Doel, S. Allam, Robert A. Gruendl, V. Scarpine, Joe Zuntz, F. Paz-Chinchón, M. Carrasco Kind, A. Carnero Rosell, A. K. Romer, M. Costanzi, J. Muir, R. L. C. Ogando, Dragan Huterer, J. P. Dietrich, Juan Garcia-Bellido, J. Annis, David J. Brooks, Jennifer L. Marshall, Ofer Lahav, E. Suchyta, J. De Vicente, A. Roodman, M. March, D. L. Hollowood, S. Serrano, S. Everett, 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, Muir, J., Bernstein, G. M., Huterer, D., Elsner, F., Krause, E., Roodman, A., Allam, S., Annis, J., Avila, S., Bechtol, K., Bertin, E., Brooks, D., Buckley-Geer, E., Burke, D. L., Carnero Rosell, A., Carrasco Kind, M., Carretero, J., Cawthon, R., Costanzi, M., da Costa, L. N., De Vicente, J., Desai, S., Dietrich, J. P., Doel, P., Eifler, T. F., Everett, S., Fosalba, P., Frieman, J., García-Bellido, J., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Hartley, W. G., Hollowood, D. L., James, D. J., Jarvis, M., Kuehn, K., Kuropatkin, N., Lahav, O., March, M., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Ogando, R. L. C., Palmese, A., Paz-Chinchón, F., Plazas, A. A., Romer, A. K., Sanchez, E., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Suchyta, E., Tarle, G., Thomas, D., Troxel, M. A., Walker, A. R., Weller, J., Wester, W., Zuntz, J., and Des, Collaboration

Subjects
Accuracy and precision, Cosmology and Nongalactic Astrophysics (astro-ph.CO), Blinding, statistical [methods], FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Cosmology, methods: numerical, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Cluster analysis, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Weak gravitational lensing, Physics, methods: statistical, 010308 nuclear & particles physics, Estimation theory, Astronomy and Astrophysics, numerical [methods], methods: data analysis, Galaxy, Space and Planetary Science, cosmology: observations, data analysi [methods], Dark energy, astro-ph.CO, large-scale structure of Universe, Astrophysics - Instrumentation and Methods for Astrophysics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Algorithm, Astrophysics - Cosmology and Nongalactic Astrophysics, observation [cosmology], astro-ph.IM
Abstract

The goal of blinding is to hide an experiment's critical results -- here the inferred cosmological parameters -- until all decisions affecting its analysis have been finalised. This is especially important in the current era of precision cosmology, when the results of any new experiment are closely scrutinised for consistency or tension with previous results. In analyses that combine multiple observational probes, like the combination of galaxy clustering and weak lensing in the Dark Energy Survey (DES), it is challenging to blind the results while retaining the ability to check for (in)consistency between different parts of the data. We propose a simple new blinding transformation that works by modifying the summary statistics that are input to parameter estimation, such as two-point correlation functions. The transformation shifts the measured statistics to new values that are consistent with (blindly) shifted cosmological parameters, while preserving internal (in)consistency. We apply the blinding transformation to simulated data for the projected DES Year 3 galaxy clustering and weak lensing analysis, demonstrating that practical blinding is achieved without significant perturbation of internal-consistency checks, as measured here by degradation of the $\chi^2$ between data and best-fitting model. Our blinding method conserves $\chi^2$ more precisely as experiments evolve to higher precision., Comment: 18 pages, 13 figures, data available upon request. Updated to match published version

Published
2020
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440. Observation and confirmation of nine strong-lensing systems in Dark Energy Survey Year 1 data

Author

M. Smith, Daniel Gruen, V. Scarpine, A. K. Romer, Felipe Menanteau, M. E. C. Swanson, Eli S. Rykoff, E. Suchyta, Enrique Gaztanaga, August E. Evrard, J. Carretero, Marco A. P. Lima, Juan Garcia-Bellido, Brian Nord, Michael Schubnell, Adriano Agnello, C. Davis, Keith Bechtol, Flavia Sobreira, Santiago Avila, M. Carrasco Kind, A. Carnero Rosell, I. Sevilla-Noarbe, Carlos E. Cunha, Yanxi Zhang, Douglas L. Tucker, Kyler Kuehn, Tim Eifler, G. Gutierrez, G. Tarle, A. A. Plazas, N. Kuropatkin, Enrique Fernández, L. N. da Costa, Huan Lin, Josh Frieman, M. March, K. Honscheid, David J. James, David J. Brooks, R. H. Schindler, Pablo Fosalba, T. M. C. Abbott, D. L. Burke, Ofer Lahav, Peter Doel, E. J. Sanchez, S. Allam, Robert A. Gruendl, Marcelle Soares-Santos, H. T. Diehl, J. Annis, D. L. Hollowood, J. De Vicente, W. G. Hartley, Jennifer L. Marshall, Daniel Thomas, E. Buckley-Geer, Adam Amara, Ramon Miquel, Thomas E. Collett, A. Roodman, B. Flaugher, Ben Hoyle, M. A. G. Maia, Peter Melchior, Department of Energy (US), National Science Foundation (US), Ministerio de Ciencia, Innovación y Universidades (España), Science and Technology Facilities Council (UK), University of Illinois, Kavli Institute for Theoretical Physics, University of Chicago, The Ohio State University, Texas A&M University, Financiadora de Estudos e Projetos (Brasil), Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico (Brasil), Ministério da Ciência, Tecnologia e Inovação (Brasil), and German Research Foundation

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), Higher education, Gravitational lensing: strong, DES [surveys], astro-ph.GA, Library science, Techniques: spectroscopic, FOS: Physical sciences, clusters [gravitational lensing], Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, survey [gravitational lensing], Galaxies: individual, 0103 physical sciences, media_common.cataloged_instance, Astrophysics::Solar and Stellar Astrophysics, European union, general [gravitational lenses], 010303 astronomy & astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Astrophysics::Galaxy Astrophysics, STFC, media_common, Physics, 010308 nuclear & particles physics, business.industry, RCUK, Astronomy and Astrophysics, Astrophysics - Astrophysics of Galaxies, gravitational lensing individual, Alliance, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), strong [gravitational lensing], Fundamental physics, astro-ph.CO, Christian ministry, business, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics, astro-ph.IM
Abstract

We describe the observation and confirmation of nine new strong gravitational lenses discovered in Year 1 data from the Dark Energy Survey (DES). We created candidate lists based on (i) galaxy group and cluster samples, and (ii) photometrically selected galaxy samples. We selected 46 candidates through visual inspection and then used the Gemini Multi-Object Spectrograph (GMOS) at the Gemini South telescope to acquire a spectroscopic follow-up of 21 of these candidates. Through an analysis of these spectroscopic follow-up data, we confirmed nine new lensing systems and rejected two candidates, and the analysis was inconclusive on 10 candidates. For each of the confirmed systems, our report measured spectroscopic properties, estimated source image-lens separations, and estimated enclosed masses as well. The sources that we targeted have an i-band surface brightness range of i ∼ 22-24 mag arcsec and a spectroscopic redshift range of z ∼ 0.8−2.6. The lens galaxies have a photometric redshift range of z ∼ 0.3−0.7. The lensing systems range in source image-lens separation from 2 to 9 arcsec and in enclosed mass from 10 to 10 M, 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, Fundac¸ão 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 e Tecnologia, the Deutsche Forschungsge-meinschaft, and the Collaborating Institutions in the DES. The DES data management system is supported by the National Science Foundation under Grant Number AST-1138766. The DES participants from Spanish institutions are partially supported by MINECO under grants AYA2012-39559, ESP2013-48274, FPA2013-47986, and Centro de Excelencia Severo Ochoa SEV-2012-0234, some of which include ERDF funds from the European Union. 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
2020
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441. Weak-lensing analysis of SPT-selected galaxy clusters using Dark Energy Survey Science Verification data

Author

F. J. Castander, R. C. Smith, Donnacha Kirk, Alistair R. Walker, Michael Schubnell, Juan Garcia-Bellido, T. M. C. Abbott, Tim Schrabback, Christian L. Reichardt, E. J. Sanchez, Rafe Schindler, D. L. Burke, Robert A. Gruendl, Marcos Lima, Joe Zuntz, M. Carrasco Kind, David J. Brooks, Shantanu Desai, J. Carretero, Tesla E. Jeltema, Bradford Benson, D. Applegate, C. Stern, Sebastian Bocquet, David Rapetti, J. De Vicente, I-Non Chiu, A. Carnero Rosell, Ofer Lahav, Sarah Bridle, Flavia Sobreira, Enrique Gaztanaga, G. Gutierrez, Michael Troxel, Erin Sheldon, D. L. Hollowood, Santiago Avila, M. E. C. Swanson, Nikhel Gupta, M. A. G. Maia, J. P. Dietrich, Filipe B. Abdalla, Felipe Menanteau, Joshua A. Frieman, C. B. D'Andrea, Kyler Kuehn, Gregory Tarle, I. Sevilla-Noarbe, M. March, N. Kuropatkin, Matt J. Jarvis, Pablo Fosalba, T. Kacprzak, L. N. da Costa, E. Suchyta, August E. Evrard, Peter Melchior, R. Capasso, Joseph J. Mohr, A. Saro, Juan Estrada, B. Flaugher, Peter Doel, A. A. Plazas, H. T. Diehl, E. Bertin, C. Davis, J. Gschwend, A. K. Romer, M. Smith, Daniel Gruen, Ramon Miquel, Benjamin Saliwanchik, 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, SPT, Institut d'Astrophysique de Paris ( IAP ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ), Stern, C., Dietrich, J. P., Bocquet, S., Applegate, D., Mohr, J. J., Bridle, S. L., Carrasco Kind, M., Gruen, D., Jarvis, M., Kacprzak, T., Saro, A., Sheldon, E., Troxel, M. A., Zuntz, J., Benson, B. A., Capasso, R., Chiu, I., Desai, S., Rapetti, D., Reichardt, C. L., Saliwanchik, Schrabback, T., Gupta, N., Abbott, T. M. C., Abdalla, F. B., Avila, S., Bertin, E., Brooks, D., Burke, D. L., Carnero Rosell, A., Carretero, J., Castander, F. J., D'Andrea, C. B., da Costa, L. N., Davis, C., De Vicente, J., Diehl, H. T., Doel, P., Estrada, J., Evrard, A. E., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hollowood, D., Jeltema, T., Kirk, D., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. A. G., March, M., Melchior, P., Menanteau, F., Miquel, R., Plazas, A. A., Romer, A. K., Sanchez, E., Schindler, R., Schubnell, M., Sevilla-Noarbe, I., Smith, M., Smith, R. C., Sobreira, F., Suchyta, E., Swanson, M. E. C., Tarle, G., Walker, A. R., Des, Collaboration, and Spt, Collaboration

Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO), [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, Cosmology, gravitational lensing: weak, weak [gravitational lensing], 0103 physical sciences, clusters: general [galaxies], LENTES GRAVITACIONAIS, 010303 astronomy & astrophysics, Weak gravitational lensing, Galaxy cluster, Physics, 010308 nuclear & particles physics, GALÁXIAS, Astronomy and Astrophysics, observations [cosmology], Redshift, South Pole Telescope, True mass, galaxies: clusters: general, Space and Planetary Science, cosmology: observations, Astrophysics - Cosmology and Nongalactic Astrophysics, Log-normal distribution, astro-ph.CO, Dark energy, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], observation [cosmology]
Abstract

We present weak lensing (WL) mass constraints for a sample of massive galaxy clusters detected by the South Pole Telescope (SPT) via the Sunyaev-Zeldovich effect (SZE). We use $griz$ imaging data obtained from the Science Verification (SV) phase of the Dark Energy Survey (DES) to fit the WL shear signal of 33 clusters in the redshift range $0.25 \le z \le 0.8$ with NFW profiles and to constrain a four-parameter SPT mass-observable relation. To account for biases in WL masses, we introduce a WL mass to true mass scaling relation described by a mean bias and an intrinsic, log-normal scatter. We allow for correlated scatter within the WL and SZE mass-observable relations and use simulations to constrain priors on nuisance parameters related to bias and scatter from WL. We constrain the normalization of the $\zeta-M_{500}$ relation, $A_\mathrm{SZ}=12.0_{-6.7}^{+2.6}$ when using a prior on the mass slope $B_\mathrm{SZ}$ from the latest SPT cluster cosmology analysis. Without this prior, we recover $A_\mathrm{SZ}=10.8_{-5.2}^{+2.3}$ and $B_\mathrm{SZ}=1.30_{-0.44}^{+0.22}$. Results in both cases imply lower cluster masses than measured in previous work with and without WL, although the uncertainties are large. The WL derived value of $B_\mathrm{SZ}$ is $\approx 20\%$ lower than the value preferred by the most recent SPT cluster cosmology analysis. The method demonstrated in this work is designed to constrain cluster masses and cosmological parameters simultaneously and will form the basis for subsequent studies that employ the full SPT cluster sample together with the DES data., Comment: Revised version in response to referee report

Published
2019
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442. Search for Higgs boson pair production in the γγbb‾ final state in pp collisions at s=13TeV

Author

André Holzner, Santeri Laurila, Faridah Mohamad Idris, Emmanuel Olaiya, Alexander Schmidt, Vytautas Dudenas, Nadir Daci, David Sheffield, Mohsen Khakzad, Suneel Dutt, Andre David Tinoco Mendes, Guido Tonelli, Zeljko Antunovic, Claudia-Elisabeth Wulz, Christoph Paus, Roberto Dell'Orso, Sergey Troshin, Meng Wang, David D'Enterria, Wolfgang Waltenberger, Piergiulio Lenzi, Arthur Moraes, Eddi A De Wolf, Davide Cieri, Jim Hanlon, Marius Teroerde, Isa Dumanoglu, Helio Nogima, K. Rose, Alberto Orso Maria Iorio, S. Seif El Nasr-storey, Andreas Hinzmann, Michael Finger Jr, Hui Li, Salvatore My, Georgia Karapostoli, Jose Chinellato, Richard Cavanaugh, Ievgen Korol, Huseyin Topakli, Gregor Mittag, Jennifer Chu, Viktor Khristenko, Jasper Lauwers, Zheng Wang, Wajid Ali Khan, Felice Pantaleo, Chanwook Hwang, Niladribihari Sahoo, Apichart Hortiangtham, Dezso Horvath, Luisa Alunni Solestizi, Ryan Mueller, W. Bertl, James Dolen, Ivan Pozdnyakov, Ruchi Chudasama, Marco Rovere, Alexander Richards, Marco Toliman Lucchini, Mauricio Thiel, Ilya Gorbunov, Daniele Bonacorsi, Marcin Konecki, Artur Lobanov, Nathaniel Pastika, Zukhaimira Zolkapli, Kyle Tos, Antonio Delgado Peris, Ioannis Evangelou, Geonhee Oh, David Romero Abad, Anne-Laure Pequegnot, Lisa Borgonovi, Adel Terkulov, Caglar Zorbilmez, Inna Kucher, Freya Blekman, Ilse Krätschmer, Stephane Perries, David Michael Morse, Andreas Güth, Peter Timothy Cox, S. Mukhopadhyay, Mikhail Danilov, Elisabetta Gallo, Vincenzo Ciriolo, Gaël Perrin, Umesh Joshi, Jason Sang Hun Lee, Thong Nguyen, Hans Van Haevermaet, Till Arndt, Shao Min Tan, Carsten Heidemann, Costas Foudas, Roberto Sacchi, Patricia Rebello Teles, Tejinder Virdee, Nicolò Tosi, Camilla Galloni, Seth Conrad Zenz, Andrew Godshalk, Vincenzo Daponte, Daniele Marconi, Julia Thom, Finn Rebassoo, Rebeca Gonzalez Suarez, Devdatta Majumder, Volker Blobel, J. 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Tsamalaidze, Nicanor Colino, Dominik Nowatschin, Franco Fabbri, Pietro Vischia, Fionn Ball, T. Tabarelli de Fatis, Joao Seixas, Francisco Matorras, Yacine Haddad, Antonio Ranieri, John A Coughlan, S. Sanchez Cruz, Mauro Menichelli, Mirena Ivova Paneva, Dominick Olivito, Thomas Eichhorn, Mar Barrio Luna, Alessandro Thea, Cristina Fernandez Bedoya, Colin Jessop, Manuel Olmedo Negrete, Isabel Pedraza, Sunil Somalwar, Saswati Nandan, Richard Vidal, Emilien Chapon, Matthias Kasemann, Thomas Strebler, Marc Osherson, Matteo Centis Vignali, Vittorio Raoul Tavolaro, D. Meister, Paola Salvini, F. Thyssen, Marcos Fernandez, J William Gary, Florian Beaudette, Marek Walczak, Marcella Diemoz, Mareike Meyer, Deniz Sunar Cerci, Laszlo Gutay, Luca Perniè, Roland Horisberger, Yuan Chao, Georgios Mavromanolakis, Michele Arneodo, Pallabi Das, Georg Steinbrück, Elisa Manoni, Brieuc Francois, L. Lloret Iglesias, Paul Edmund Karchin, Thomas Madlener, Christopher Rogan, Alexander Dermenev, Dong Ho Moon, Seyyed Mohammad Amin Ghiasi Shirazi, Nikolai Krasnikov, Sami Lehti, Adish Vartak, Valentina Mariani, Andrew Hart, Demetrios Loukas, Jan Kieseler, Giulia Negro, Simon De Visscher, Mithat Kaya, Giorgia Rauco, Suyong Choi, Etiennette Auffray, Maurizio Biasini, Sinan Sagir, Marta Felcini, Mark Derdzinski, Daniel Tapia Takaki, Pawan Kumar Netrakanti, Petar Adzic, Maria Margherita Obertino, Alajos Makovec, Muhammad Gul, Engin Eren, Michele Gallinaro, F. Drouhin, Junquan Tao, Giorgia Miniello, Peter Wittich, Francesco Fabozzi, Michal Olszewski, Chad Flores, Stefaan Tavernier, Diego Ciangottini, Johannes Grossmann, Byung-Sik Hong, Krishna Thapa, Stefano Casasso, Michael Hildreth, Oscar Gonzalez Lopez, Tanmay Sarkar, Matthew Joyce, David Petyt, Hans Rykaczewski, Gian Piero Siroli, Metin Yalvac, Stephan Lammel, Tagir Aushev, Hugo Delannoy, Daniel Noonan, Salim Cerci, Olaf Behnke, Kyong Sei Lee, Evgueni Vlasov, Enrico Robutti, Ruslan Chistov, Kadri Ozdemir, Tirso Alejandro Gómez Espinosa, Heriberto Castilla-Valdez, Adam Dishaw, Claudia Seitz, Shin-Shan Yu, Nikitas Loukas, Mani Tripathi, Rachel Bartek, Marco Peruzzi, Usama Hussain, Owen Rosser Long, Warren Clarida, Cesare Calabria, Nicola Amapane, Matteo Sani, Andreas Nowack, Andrew Ackert, Elif Asli Yetkin, Koushik Mandal, Paraskevas Sphicas, Pierre Van Mechelen, Alberto Benvenuti, Maria Agnese Ciocci, Dave Pellett, Marko Kovac, Maria Florencia Canelli, Fabrizio Ferro, Thomas Ferbel, Dan Green, R. I. Rabadan-Trejo, Marta Ruspa, Stepan Obraztsov, Gabriella Pugliese, Valerio Calvelli, C. Mesropian, Kevin Lannon, Kenyi Hurtado Anampa, Guenakh Mitselmakher, Jordan Damgov, Shawn Williamson, D. Di Croce, S. Lisniak, Bora Akgun, Peter Hansen, Ivan Shvetsov, Igor Golutvin, Mircho Rodozov, Maria Aldaya Martin, Jennifer Ngadiuba, Jay Mathew Lawhorn, Claude Amsler, Zhoudunming Tu, Kurtis F Johnson, Laurent Favart, Cristian Pena, Thomas Reis, Martin Lipinski, Frank Würthwein, Jordi Duarte Campderros, Manas Maity, Alexi Mestvirishvili, Ulrich Goerlach, Joze Zobec, Merijn Van De Klundert, Steve Nahn, M. A. Harrendorf, Paolo Capiluppi, James Rohlf, Carlos Avila, Akram Khan, Luigi Guiducci, Gregory R Snow, Sergei Bitioukov, Jared Turkewitz, Igor Volobouev, Nicolas Chanon, Helena Malbouisson, Alex J. Barker, Barbara Clerbaux, Ricardo Eusebi, Greg P Heath, W. J. Womersley, Chiara Mariotti, Houmani El Mamouni, Marco Monteno, Alexey Kalinin, W. Wu, Nicola Bacchetta, Alexey Volkov, Attila Racz, Roberta Arcidiacono, Christian Schnaible, Jonathan Fulcher, Anatoli Pashenkov, Mikhail Ignatenko, Jelena Luetic, Tapio Lampén, Maxime Gouzevitch, Andrea Beschi, Camelia Mironov, Jeongeun Lee, Georg Sieber, Ilknur Hos, Alessio Boletti, Jie Zhang, Ewerton Belchior Batista Das Chagas, Marek Niedziela, J. N. Butler, Fabiola Vazquez Valencia, Christoph Schäfer, Marcello Maggi, Davide Piccolo, Francesca Romana Cavallo, Vincenzo Monaco, Cristina Tuve, Humberto Antonio Salazar Ibarguen, Julie Malcles, Fengwangdong Zhang, Fabrizio Fabbri, Rosamaria Venditti, Anastasia Karavdina, Bożena Boimska, Kerem Cankocak, Geum Bong Yu, Harrison Prosper, Claudia Cecchi, Christoph Wissing, Norraphat Srimanobhas, Riccardo Di Maria, Dermot Moran, Giovanni Zevi Della Porta, Viktor Savrin, Mitchell Wayne, Karol Bunkowski, Sandeep Kaur, Natale Demaria, Alexander Grohsjean, Yueh-Feng Liu, Yi-ting Duh, S. Baffioni, Tanvi Wamorkar, Carsten Hensel, Genius Walia, Paolo Lariccia, Dmitry Sosnov, Rudolf Fruehwirth, Nick Van Remortel, Chad Freer, Stefan Piperov, Boris Grynyov, Dimitrios Tsitsonis, Peter Thomassen, Phillip Russell Dudero, Shengquan Tuo, Abhigyan Dasgupta, Giorgio Maggi, Sadia Khalil, T. Mäenpää, Nikolai Skatchkov, Louis Antonelli, Seth Cooper, Can You, Walter Van Doninck, Bahareh Roozbahani, Stefan Grünendahl, Amedeo Staiano, Michael Albrow, Semra Turkcapar, Robert Schöfbeck, Linda Finco, Alfredo Castaneda Hernandez, Marta Baselga, Stephen Robert Wagner, Bhawandeep Bhawandeep, Young Ho Shin, Rostyslav Shevchenko, Sudeshna Banerjee, Lev Uvarov, Andreas Werner Jung, Rajdeep Mohan Chatterjee, Vladimir Andreev, Hamed Bakhshiansohi, Antonio Morelos Pineda, Stephan Linn, Alexander Dierlamm, Minna Leonora Vesterbacka Olsson, V. Zhukov, Mingshui Chen, Marguerite Tonjes, David Mark Raymond, Olivier Bondu, Esteban Curras, Christophe Delaere, Jose Monroy, K. Goulianos, Philip Harris, Noemi Beni, Stilianos Kesisoglou, Rocio Vilar Cortabitarte, Miroslav Finger, Borislav Pavlov, Pablo Martinez Ruiz del Arbol, Victor Kim, Ramandeep Kumar, Aruna Nayak, Michael Plagge, Csaba Hajdu, Emyr Clement, K. Pauwels, Willem Verbeke, Armando Lanaro, Gervasio Gomez, Daniel Bloch, Cameron Bravo, Matthias Komm, Arnab Purohit, Olivér Surányi, Scott Thomas, Piero Giorgio Verdini, Y. Pakhotin, Javier Fernandez Menendez, Maria Isabel Josa, Sungwoong Cho, Daniele Pedrini, Benedikt Maier, Konrad Deiters, T. Esch, Michal Szleper, Philippe Gras, Roberto Chierici, Chia-Ming Kuo, Jack Wright, Edgar Carrera Jarrin, Giuseppe Benedetto Cerati, Luis Junior Sanchez Rosas, Konstantin Androsov, Tai Sakuma, Shashikant Dugad, Kevin Deroover, Candan Dozen, Michael Wayne Arenton, Sean Kalafut, Stavros Mallios, Johannes Wittmann, James D. Olsen, Archana Sharma, Matevz Tadel, Daniel Salerno, Aobo Zhang, Xuyang Gao, Olena Karacheban, Cristóvão Beirão Da Cruz E Silva, Viola Sordini, Erika Garutti, Eva Halkiadakis, Fred-Markus Helmut Stober, Manuel Franco Sevilla, Shirin Chenarani, Jian Sun, Jozsef Molnar, Valerio Re, S. Liu, Clemencia Mora Herrera, Mario Masciovecchio, Frank Glege, Iurii Antropov, Stefano Marcellini, Huilin Qu, Lieselotte Moreels, Shalini Thakur, James John Brooke, Cédric Prieels, Martina Ressegotti, Rohan Bhandari, Vinay Hegde, Saptaparna Bhattacharya, A. Degano, David Zou, Andrey Korytov, P. Chang, Gérald Grenier, Eduardo De Moraes Gregores, Fabrizio Gasparini, Michele Selvaggi, Artur Kalinowski, Junho Kim, Deborah Duchardt, Marco Verzocchi, Luigi Benussi, Gouranga Kole, Anterpreet Kaur, Bruno Galinhas, Alessandro Braghieri, Johannes Schulz, Yutaro Iiyama, Intae Yu, Gregory Rakness, Giancarlo Mantovani, Carlo Battilana, Sezen Sekmen, P. Lujan, Charles Ferraioli, Pooja Saxena, Roger Rusack, Marc Dejardin, Tielige Mengke, Ashfaq Ahmad, Irving Daniel Sandoval Gonzalez, Gulsen Onengut, Viktor Matveev, Ashim Roy, Clemens Lange, Santiago Folgueras, George Alverson, Roman Kogler, Benjamin Kreis, Myriam Schönenberger, A. Tatarinov, Irene Dutta, Johannes Hauk, Antonio María Pérez-Calero Yzquierdo, Young Do Oh, Daniel Gonzalez, Mark Pesaresi, James Letts, Ravi Janjam, Siddharth Narayanan, Anton Karneyeu, Leonard Apanasevich, Weinan Si, John Wood, Jung-Hyun Kim, Anna Elliott-Peisert, Jan Krolikowski, Luiz Mundim, Vuko Brigljevic, Dmitry Philippov, Duccio Abbaneo, David Taylor, Elizabeth Locci, Ilaria Vai, Frank Hartmann, Luciano Orsini, Markus Seidel, Jochen Schieck, Vineet Kumar, Gabriele Benelli, Patrizia Barria, R. Ciesielski, Somnath Choudhury, Claus Kleinwort, Alexander Savin, Luca Pacher, Vasile Mihai Ghete, Troy Mulholland, James Castle, Claire Shepherd-Themistocleous, Seungkyu Ha, Christian Barth, Daniele Fasanella, Antonis Agapitos, Thi Hien Doan, Daniel Denegri, Charalambos Nicolaou, Aran Garcia-Bellido, Franco Ligabue, F. Giordano, Niki Saoulidou, Zhengcheng Tao, Hartmut Stadie, Natascha Krammer, James Zabel, Adrian Byszuk, Kenneth Long, Andre Govinda Stahl Leiton, Zhenyu Chen, Andrea Carlo Marini, Roberto Rossin, Alexander Tapper, Vyacheslav Krutelyov, Paul Kyberd, Sema Zahid, Nikoloz Skhirtladze, Geoffrey Smith, Sergei Gleyzer, Ana Ovcharova, Andrea Venturi, Muhammad Shoaib, M. Jo, Luisa Fernanda Chaparro Sierra, Deborah Pinna, Caterina Vernieri, Bo Liu, Giuseppe Codispoti, Mia Tosi, Ta-Wei Wang, Piet Verwilligen, Stefan Spanier, Brian Dorney, Prashant Shukla, Cristina Oropeza Barrera, Mariarosaria D'Alfonso, Mario Galanti, Zoltan Szillasi, André Rosowsky, Andrew Ivanov, Andrey Uzunian, Christopher Palmer, Annika Vanhoefer, Alice Bean, David Yu, A. Caudron, Balazs Ujvari, Yuri Musienko, Francesco Fienga, Shervin Nourbakhsh, Monica Vazquez Acosta, Andrzej Pyskir, Arsen Khvedelidze, Joachim Mnich, Qiang Li, Nabarun Dev, Viacheslav Bunichev, Johan Borg, Naimuddin, Rafael Teixeira De Lima, Thomas Lenzi, Min Suk Kim, Fotios Ptochos, Manfred Paulini, Pierluigi Bortignon, Charles Harrington, Ugo Gasparini, Veikko Karimäki, Maximilian Heindl, Nicola Cavallo, Sara Fiorendi, Allison Reinsvold, Vasken Hagopian, Bhargav Madhusudan Joshi, Riccardo Bellan, Zeynep Demiragli, Yalcin Guler, Roger Wolf, Lev Dudko, Jeremy Andrea, Joseph Heideman, Marta Verweij, Pierluigi Zotto, Suresh C Tonwar, Sylvie Braibant-Giacomelli, Hwi Dong Yoo, Zijun Xu, Robert Bainbridge, V. Knünz, Gobinda Majumder, Stefano Ragazzi, Jane Nachtman, Sean-Jiun Wang, Claudio Grandi, Sergio F Novaes, Samet Lezki, R. Reyes-Almanza, Morgan Lethuillier, Yasar Onel, Sébastien Gadrat, Mayda Velasco, Jonatan Piedra Gomez, M. Melo De Almeida, Ignacio Redondo, Benjamin Stieger, Hyun-Chul Kim, Yurii Maravin, Vladimir Gavrilov, Aleko Khukhunaishvili, Sonaina Undleeb, Igor Miagkov, T. Matsushita, Hannes Jung, Alexander Zhokin, Martijn Mulders, Tao Huang, Sushil Chauhan, Anna Colaleo, Kamal Lamichhane, Mary Hadley, Martino Margoni, Alexander Spiridonov, Francesca Nessi-Tedaldi, Ron Lipton, Anadi Canepa, Dario Menasce, Michael Krohn, Jeremie Alexandre Merlin, Piotr Zalewski, Xinmei Niu, Simranjit Singh Chhibra, Eric Conte, David Barney, Aleksandra Lelek, Stephanie Beauceron, Joshua Kunkle, Mark Raymond Adams, Ulrich Husemann, B. Michlin, Valentina Sola, Vitaly Smirnov, Dragos Velicanu, Qamar Hassan, Sudhir Malik, Ia Iashvili, Monoranjan Guchait, Fabio Colombo, Jean-Roch Vlimant, Brajesh C Choudhary, Paul David Luckey, Marco Trovato, Sébastien Viret, Nuno Leonardo, Ashutosh Bhardwaj, Kelly Beernaert, Eric Wayne Vaandering, Yagya Raj Joshi, Susan Gascon, Stefano Colafranceschi, Siarhei Shulha, Paolo Gunnellini, Batool Safarzadeh, Juliet Ritchie Patterson, Gunther Roland, Joao Varela, Illia Khvastunov, Bipen Singh, Leander Litov, Peter Raics, Peicho Petkov, Michele De Gruttola, Jean-Pierre Merlo, Leonardo Cristella, Lea Caminada, Achille Petrilli, Chun-Hua Jiang, Rocky Bala Garg, Joanne Cole, Eija Tuominen, Luigi Fiore, Patrick Connor, Roberval Walsh, Giovanna Selvaggi, Daniel Abercrombie, Gagan Bihari Mohanty, Simon Regnard, Gabor Istvan Veres, Alexandre Mertens, Sarah Catherine Eno, Jan-Frederik Schulte, Sourav Dey, Leonid Levchuk, Luca Scodellaro, Christos Roskas, Isis Van Parijs, Maria Cepeda, Jorgen D'Hondt, Hugues Brun, Pieter Everaerts, Titas Roy, Olga Kodolova, Alexx Perloff, Roman Ryutin, Federica Primavera, Roberto Carlin, Pierre Depasse, Vyacheslav Klyukhin, Kajari Mazumdar, Nickolas Mccoll, Nadeesha Wickramage, Anna Zanetti, Salvatore Buontempo, Dustin Stolp, Lorenzo Viliani, Kurt Jung, Paul Avery, Salavat Abdullin, Lisa Benato, Gino Bolla, Isabelle De Bruyn, Quentin Python, Randy Ruchti, Joe Incandela, Luca Cadamuro, Virginia Azzolini, Mateusz Zarucki, Dan Quach, Marcus Hohlmann, Rylan Conway, Matthias Ulrich Mozer, H. Neugebauer, Carlos Florez, Nataliia Kovalchuk, Johannes Brandstetter, Alexander Malakhov, Efe Yazgan, Günter Flügge, Qiao Xu, Tyler Ruggles, B. Tali, Robert Clare, Patrizia Azzi, Hannes Sakulin, Thomas Hebbeker, Paul Lecoq, Tilman Rohe, Jing Wang, Laura Dodd, Ksenia Shchelina, Albert M. Sirunyan, Andrew Levin, Anton Stepennov, Chiara Amendola, Alexandre Zabi, Marino Missiroli, Ashley Parker, Andrius Juodagalvis, Anshul Kapoor, Vladimir Karjavin, Kerstin Borras, Eduard De La Cruz-Burelo, Juan Manuel Grados Luyando, Ka Hei Martin Kwok, Andrew Evans, Dong-Chul Son, Liliana Teodorescu, Adolf Bornheim, Aaron Bundock, Frans Meijers, F. Cenna, Katerina Lipka, Martin Kirakosyan, Filippo Errico, Bodhitha Jayatilaka, Jean-Louis Faure, Philipp Millet, Gerrit Patrick Van Onsem, Ivan Heredia-De La Cruz, Howard Wells Wulsin, Clément Leloup, Alexander Nikitenko, Edward Scott, Kristian Harder, T. Lomtadze, P. Hebda, Jasvinder A. Singh, Vladimir Petrov, Thomas N. Williams, Brian Francis, Paolo Checchia, Zhixing Wang, Dipanwita Dutta, Stefan Wayand, Alexei Safonov, Alberto Messineo, John Almond, Janos Erö, William Mcbrayer, José Cupertino Ruiz Vargas, Julia Velkovska, Simone Paoletti, Suchandra Dutta, Giulio Mandorli, Anne-Marie Magnan, Wagner Carvalho, Sudha Ahuja, Halil Saka, Pietro Govoni, Maryam Zeinali, Patrick Jarry, Benjamin Charles Radburn-Smith, Kevin Nash, Hongbo Liao, Terhi Jarvinen, Greg Landsberg, Cécile Caillol, Giuseppe Della Ricca, Sw. Banerjee, L. Brito, Asif Saddique, Alessandro Rossi, Matthias Schröder, Valentina Dutta, M. Hoffmann, Kyungwook Nam, Bobak Hashemi, Alice Magnani, Manjit Kaur, Tom Cornelis, Shivali Malhotra, Gunter Quast, Tanmay Mudholkar, Ennio Monteil, Aldo Penzo, Nicolas Tonon, Vladimir Popov, Matteo Cremonesi, Jaehoon Lim, Nitish Dhingra, Satoshi Hasegawa, Samuel Bein, Daniel Spitzbart, Michail Bachtis, Francesco Fiori, Yildiray Komurcu, Philippe Busson, Andreas Psallidas, Dipak Kumar Sahoo, Douglas Wright, Giacomo Fedi, Nikkie Deelen, Alice Cocoros, Panagiotis Katsoulis, Stephen Mrenna, Denys Lontkovskyi, Afiq Aizuddin Bin Anuar, Marc Weinberg, Marco Zanetti, Tae Jeong Kim, Duncan Carlsmith, John Hakala, Michael Murray, Jakob Salfeld-Nebgen, Fatma Boran, Prakash Thapa, Nazar Bartosik, Enrique Palencia Cortezon, Marvin Johnson, Marco De Mattia, N. Terentyev, C. A. Carrillo Montoya, Silvia Goy Lopez, Zoltan Gecse, Jongseok Lee, Pedrame Bargassa, Hasan Ogul, Nick Amin, Aram Apyan, Nikolay Voytishin, Andreas Künsken, Laurent Thomas, Olivier Davignon, Dmitri Konstantinov, R. Fischer, John Perry Cumalat, Swagata Mukherjee, Valentin Sulimov, Philip H Butler, Prolay Mal, Toni Sculac, Inkyu Park, Oliver Gutsche, F. Scheuch, Javier Martin Blanco, Douglas Burns, Francisco Yumiceva, Andreas Pfeiffer, Kreso Kadija, Jeffrey Richman, Gilvan Alves, Hyunyong Kim, J. f. Tsai, Kira Burt, Kirill Skovpen, Victor Murzin, Ritva Kinnunen, Petar Maksimovic, Patrick Janot, Thorsten Chwalek, Matthew Carver, Merve Nazlim Agaras, Mehar Ali Shah, Miaoyuan Liu, Gustavo Gil Da Silveira, Tutanon Sinthuprasith, Navid Rad, Katja Klein, Geng-Yuan Jeng, A. Borzou, Irene Bachiller, Pieter David, Cristina Biino, Ivan Mikulec, Nathaniel Woods, Francesco Micheli, Gul Gokbulut, Savvas Kyriacou, Denis Rathjens, Raghav Kunnawalkam Elayavalli, Markus Radziej, Dylan Gilbert, Georgios Krintiras, Tobias Pook, Jay Hauser, Andrei Starodumov, Isidro Gonzalez Caballero, Florian Kassel, Michael Brodski, Roberto Castello, Elizabeth Sexton-Kennedy, Matthias Wolf, Paolo Ronchese, Badder Marzocchi, Sanjay Kumar Swain, Marc M Baarmand, Daniele Trocino, Silvia Maselli, Winston Ko, Reza Goldouzian, Mohd Nizam Yusli, Renato Potenza, Guenter Eckerlin, Armen Tumasyan, Paula Eerola, Manoj Sharan, Alexis Fagot, Zhicai Zhang, Rui Xiao, Evangelos Paradas, Y. Yilmaz, Kevin Burkett, Kisoo Lee, Lalit Mohan Pant, Aaron Dominguez, Abdollah Mohammadi, P. Juillot, Walter Luiz Aldá Júnior, Felicitas Pauss, Celso Martinez Rivero, Austin Baty, Paolo Giacomelli, Wenxing Fang, Geoffrey Hall, Sanjay Padhi, Panagiotis Kokkas, Oleksandr Zenaiev, Niels Dupont, Riccardo Del Burgo, Sarah Malik, Edward Laird, Aurore Savoy-Navarro, Luca Mastrolorenzo, Vieri Candelise, Lana Beck, Ted Kolberg, Claude Charlot, Reddy Pratap Gandrajula, Ibrahim Soner Zorbakir, G. Ramirez-Sanchez, Alexandra Carvalho Antunes De Oliveira, David Vannerom, Catherine Vander Velde, Elvire Bouvier, Giuseppe Iaselli, Georgi Sultanov, Armando Bermúdez Martínez, Evan Wolfe, David Cutts, Gian Luca Pinna Angioni, Kevin Stenson, Achim Stahl, Predrag Cirkovic, M. Mohammadi Najafabadi, Daniel Troendle, Panja-Riina Luukka, Roberto Salerno, Scarlet Norberg, Ram Krishna Dewanjee, Rafael Lopes De Sá, Daniel Winterbottom, A. K. Mohanty, Po-Hsun Chen, Stefano Mersi, Mate Csanad, Ketino Kaadze, and Christian Contreras-Campana

Subjects
Physics, Nuclear and High Energy Physics, Particle physics, Photon, Luminosity (scattering theory), Large Hadron Collider, 010308 nuclear & particles physics, Branching fraction, High Energy Physics::Phenomenology, 01 natural sciences, Standard Model, Pair production, 0103 physical sciences, Higgs boson, High Energy Physics::Experiment, 010306 general physics, Boson
Abstract

A search is presented for the production of a pair of Higgs bosons, where one decays into two photons and the other one into a bottom quark-antiquark pair. The analysis is performed using proton-proton collision data at root s = 13 TeV recorded in 2016 by the CMS detector at the LHC, corresponding to an integrated luminosity of 35.9 fb(-1) . The results are in agreement with standard model (SM) predictions. In a search for resonant production, upper limits are set on the cross section for new spin-0 or spin-2 particles. For the SM-like nonresonant production hypothesis, the data exclude a product of cross section and branching fraction larger than 2.0 fb at 95% confidence level (CL), corresponding to about 24 times the SM prediction. Values of the effective Higgs boson self-coupling K X are constrained to be within the range -11 < K-lambda < 17 at 95% CL, assuming all other Higgs boson couplings are at their SM value. The constraints on K-lambda, are the most restrictive to date. (C) 2018 The Author(s). Published by Elsevier B.V.

Published
2019
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443. Slice Allocation and Pricing Framework for Virtualized Millimeter Wave Cellular Networks

Author

Juan Garcia-Rois, Felipe Gil-Castineira, Jinsong Wu, Francisco J. González-Castaño, and Beatriz Lorenzo

Subjects
Matching (statistics), General Computer Science, Computer science, media_common.quotation_subject, Context (language use), computer.software_genre, Outcome (game theory), Scarcity, Base station, pricing, Market price, Common value auction, General Materials Science, Resource management, media_common, Auctions, business.industry, infrastructure slicing, General Engineering, millimeter wave, Virtualization, 3325.08 Teléfono, matching games, Cellular network, 3325 Tecnología de las Telecomunicaciones, lcsh:Electrical engineering. Electronics. Nuclear engineering, business, lcsh:TK1-9971, computer, Computer network
Abstract

Traditionally, the cellular spectrum is allocated to operators (OPs) through auctions, as ideal mechanisms to discover market prices and allocate scarce resources. Even though spectrum is indeed scarce in sub-6 GHz bands, it becomes abundant in millimeter-wave (mmWave) bands. Interestingly, in that context, it is base station (BS) density which is limiting, and thus a critical factor, due to the outage phenomena in urban environments. Facing BS scarcity is one of the main reasons to foster virtualization techniques aimed at improving utilization and lowering costs. We consider a scenario with an infrastructure provider (InP) owner of a number of BSs and a set of OPs with their users (UEs). We propose a three-phase framework to price network infrastructure slices (NISs) and allocate them to OPs and to efficiently associate UEs with those NISs. The framework stages are: 1) an initial association, 2) a distributed auction mechanism across the BSs to allocate resources to Ops, and 3) a re-association process where the OPs can optimize the NISs they are awarded. The auction incentivizes OPs to bid truthfully and the outcome yields both socially optimal NISs and Vickrey-Clarke-Groves (VCG) prices. For the re-association phase, we propose deterministic and stochastic exchange-matching algorithms and demonstrate their convergence to stable matching and stable-optimal matching, respectively. Ministerio de Economía, Industria y Competitividad | Ref. TEC2016-76465-C2-2-R Xunta de Galicia | Ref. GRC 2018/53

Published
2019
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444. A Survey on Reversible Watermarking for Multimedia Content: A Robustness Overview

Author

Claudia Feregrino-Uribe, Rogelio Hasimoto-Beltran, Alejandra Menendez-Ortiz, and Jose Juan Garcia-Hernandez

Subjects
General Computer Science, Computer science, Digital content, 0211 other engineering and technologies, ComputingMilieux_LEGALASPECTSOFCOMPUTING, 02 engineering and technology, robustness, computer.software_genre, Reduction (complexity), Robustness (computer science), 0202 electrical engineering, electronic engineering, information engineering, General Materials Science, Digital watermarking, 021110 strategic, defence & security studies, Multimedia, Point (typography), business.industry, reversible watermarking, multimedia content, General Engineering, 020207 software engineering, Embedding, The Internet, lcsh:Electrical engineering. Electronics. Nuclear engineering, business, Host (network), computer, lcsh:TK1-9971
Abstract

In recent years, the growth of the Internet along with multimedia data delivery, have caused the misuse and even alteration of the original digital content. As a security mechanism, digital watermarking has been used to protect digital content, traditionally in copyright protection applications, and more recently digital watermarking has been used in content enhancement applications. Regardless of the application, digital watermarking schemes always cause some level of signal degradation. There are however, certain applications as in the military or medical fields, where loss of information cannot be tolerated during the reconstruction of host signals, therefore conventional watermarking schemes do not satisfy the quality requirements. In order to reconstruct signals without loss of data, reversible watermarking is employed. Recent research in reversible watermarking has focused on either, the improvement of embedding capacity or the reduction of perceptual impact of the schemes, but scarcely exploring the robustness of reversible schemes. In this survey, we provide a deep review of reversible watermarking schemes and propose a new classification outline based on the robustness point of view. Finally, some future directions for reversible watermarking research are presented and open problems in robust reversible watermarking are outlined.

Published
2019

445. Monte Carlo control loops for cosmic shear cosmology with DES Year 1 data

Author

L. F. Secco, G. Tarle, Sarah Bridle, Santiago Avila, David J. Brooks, M. A. G. Maia, S. Desai, M. Carrasco Kind, David J. James, Claudio Bruderer, G. Gutierrez, M. E. C. Swanson, Raphael Sgier, Jörg Herbel, Robert A. Gruendl, Matt J. Jarvis, W. G. Hartley, Vinu Vikram, E. Suchyta, Ben Hoyle, Juan Garcia-Bellido, J. Carretero, Adam Amara, V. Scarpine, E. Buckley-Geer, Alexandre Refregier, Peter Doel, M. Smith, Daniel Gruen, H. T. Diehl, I. Sevilla-Noarbe, L. N. da Costa, E. Bertin, Ramon Miquel, Joe Zuntz, A. A. Plazas, J. Gschwend, Marcos Lima, T. Kacprzak, Enrique Gaztanaga, Jochen Weller, J. De Vicente, E. J. Sanchez, F. Paz-Chinchón, D. L. Hollowood, S. Serrano, Andrina Nicola, Felipe Menanteau, Alex Drlica-Wagner, J. Annis, F. Tarsitano, Peter Melchior, Jennifer L. Marshall, A. Carnero Rosell, K. Honscheid, UAM. Departamento de Física Teórica, National Science Foundation (US), Science and Technology Facilities Council (UK), Department of Energy (US), German Research Foundation, Ministerio de Economía y Competitividad (España), Agencia Estatal de Investigación (España), Ministerio de Ciencia, Innovación y Universidades (España), European Commission, 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
Point spread function, Software_OPERATINGSYSTEMS, Cosmology and Nongalactic Astrophysics (astro-ph.CO), ComputingMethodologies_SIMULATIONANDMODELING, Monte Carlo method, FOS: Physical sciences, Data_CODINGANDINFORMATIONTHEORY, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, 7. Clean energy, Cosmology, Parameter Contraints, cosmic rays, 0103 physical sciences, Hardware_INTEGRATEDCIRCUITS, Experiments in gravity, Weak, 010306 general physics, Weak gravitational lensing, STFC, Gravitational Lensing, Physics, COSMIC cancer database, Code, 010308 nuclear & particles physics, Power Spectra, Física, Spectral density, RCUK, ComputerSystemsOrganization_PROCESSORARCHITECTURES, Galaxies, Dark Energy, Accurate Halo-Model, Redshift, Computational physics, Vlt Deep Survey, 13. Climate action, Dark energy, astro-ph.CO, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], cosmology, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

DES Collaboration: et al., Weak lensing by large-scale structure is a powerful probe of cosmology and of the dark universe. This cosmic shear technique relies on the accurate measurement of the shapes and redshifts of background galaxies and requires precise control of systematic errors. Monte Carlo control loops (MCCL) is a forward modeling method designed to tackle this problem. It relies on the ultra fast image generator (UFig) to produce simulated images tuned to match the target data statistically, followed by calibrations and tolerance loops. We present the first end-to-end application of this method, on the Dark Energy Survey (DES) Year 1 wide field imaging data. We simultaneously measure the shear power spectrum Cℓ and the redshift distribution n(z) of the background galaxy sample. The method includes maps of the systematic sources, point spread function (PSF), an approximate Bayesian computation (ABC) inference of the simulation model parameters, a shear calibration scheme, and a fast method to estimate the covariance matrix. We find a close statistical agreement between the simulations and the DES Y1 data using an array of diagnostics. In a nontomographic setting, we derive a set of Cℓ and n(z) curves that encode the cosmic shear measurement, as well as the systematic uncertainty. Following a blinding scheme, we measure the combination of Ωm, σ8, and intrinsic alignment amplitude AIA, defined as S8DIA=σ8(Ωm/0.3)0.5DIA, where DIA=1−0.11(AIA−1). We find S8DIA=0.895+0.054−0.039, where systematics are at the level of roughly 60% of the statistical errors. We discuss these results in the context of earlier cosmic shear analyses of the DES Y1 data. Our findings indicate that this method and its fast runtime offer good prospects for cosmic shear measurements with future wide-field surveys., 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, 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 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. ESP2015-66861, No. FPA2015-68048, No. SEV-2016-0588, No. SEV2016-0597, 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) e-Universe (CNPq grant No. 465376/2014-2).

Published
2020
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446. 22% Efficiency Inverted Perovskite Photovoltaic Cell Using Cation-Doped Brookite TiO

Author

Xiaowen, Hu, Chang, Liu, Zhiyong, Zhang, Xiao-Fang, Jiang, Juan, Garcia, Colton, Sheehan, Lingling, Shui, Shashank, Priya, Guofu, Zhou, Sen, Zhang, and Kai, Wang

Subjects
high efficiency, Communication, inverted perovskite solar cells, durability, interface engineering, Communications
Abstract

Simultaneously achieving high efficiency and high durability in perovskite solar cells is a critical step toward the commercialization of this technology. Inverted perovskite photovoltaic (IP‐PV) cells incorporating robust and low levelized‐cost‐of‐energy (LCOE) buffer layers are supposed to be a promising solution to this target. However, insufficient inventory of materials for back‐electrode buffers substantially limits the development of IP‐PV. Herein, a composite consisting of 1D cation‐doped TiO2 brookite nanorod (NR) embedded by 0D fullerene is investigated as a top modification buffer for IP‐PV. The cathode buffer is constructed by introducing fullerene to fill the interstitial space of the TiO2 NR matrix. Meanwhile, cations of transition metal Co or Fe are doped into the TiO2 NR to further tune the electronic property. Such a top buffer exhibits multifold advantages, including improved film uniformity, enhanced electron extraction and transfer ability, better energy level matching with perovskite, and stronger moisture resistance. Correspondingly, the resultant IP‐PV displays an efficiency exceeding 22% with a 22‐fold prolonged working lifetime. The strategy not only provides an essential addition to the material inventory for top electron buffers by introducing the 0D:1D composite concept, but also opens a new avenue to optimize perovskite PVs with desirable properties., A composite consisting of 1D cation‐doped TiO2 brookite nanorod embedded by 0D fullerene is investigated as a top modification buffer for inverted perovskite photovoltaic (IP‐PV) cells. The resultant IP‐PV displays an efficiency exceeding 22% with a favorable stability. This work opens up more opportunities in expanding the material inventory for charge transfer layer in perovskite solar cells development and application.

Published
2020

447. Perovskite@Graphene Nanohybrids for Breath Analysis: A Proof-of-Concept

Author

Enginyeria Electrònica, Elèctrica i Automàtica, Universitat Rovira i Virgili, Casanova-Chafer, Juan; Garcia-Aboal, Rocio; Atienzar, Pedro; Bittencourt, Carla; Llobet, Eduard, Enginyeria Electrònica, Elèctrica i Automàtica, Universitat Rovira i Virgili, and Casanova-Chafer, Juan; Garcia-Aboal, Rocio; Atienzar, Pedro; Bittencourt, Carla; Llobet, Eduard

Abstract

Nanohybrids comprising graphene loaded with perovskite nanocrystals have been demonstrated as a potential option for sensing applications. Specifically, their combination presents an interesting synergistic effect owing to greater sensitivity when bare graphene is decorated with perovskites. In addition, since the main drawback of perovskites is their instability towards ambient moisture, the hydrophobic properties of graphene can protect them, enabling their use for ambient monitoring, as previously reported. However not limited to this, the present work provides a proof-of-concept to likewise employ them in a potential application as breath analysis for the detection of health-related biomarkers. There is a growing demand for sensitive, non-invasive, miniaturized, and inexpensive devices able to detect specific gas molecules in human breath. Sensors gathering these requirements may be employed as a screening tool for reliable and fast detection of potential health issues. Moreover, perovskite@graphene nanohybrids present additional properties highly desirable as the capability to be operated at room temperature (i.e., reduced power consumption), reversible interaction with gases (i.e., reusability), and long-term stability. Within this perspective, the combination of both nanomaterials, perovskite nanocrystals and graphene, possibly includes the main requirements needed, being a promising option to be employed in the next generation of sensing devices.

Published
2021

448. LINC-21. PROGNOSTIC FACTORS AND SURVIVAL OF LOW-GRADE GLIOMAS IN CHILDREN AND ADOLESCENTS – A MULTICENTER STUDY IN PERU

Author

Rosdali Diaz-Coronado, Eddy Hernández-Broncano, Sandro Casavilca-Zambrano, Danny Campos-Sanchez, Ivan Maza, Mariela Tello, Esmeralda Leon, Hernan Cañari, Javier Custodio, Luis Ojeda-Medina, Tatiana Negreiros, Olga Cordova, Pamela Mora-Alferez, Juan Garcia-Leon, Liliana Vasquez, Daniel Moreira, and Ibrahim Qaddoumi

Subjects
Cancer Research, Oncology, Neurology (clinical)
Abstract

BACKGROUND: Low-grade gliomas (LGG) are the most common central nervous system (CNS) tumors in children. Peru is an index country for the Global Initiative for Childhood Cancer (GICC). As part of the Initiative, a multidisciplinary brain tumor team was formed in 2020 that includes five national reference centers: National Institute of Neoplastic Diseases, National Children’s Health Institute-San Borja, National Children’s Health Institute-Breña, Edgardo Rebagliati Martins National Hospital and Guillermo Almenara Irigoyen National Hospital. This multicenter study sought to evaluate the survival and prognostic factors of patients younger than 18 years diagnosed with LGG, an index cancer for the GICC. METHODS: A retrospective study included all patients diagnosed with LGG in the five centers between 2014 and 2018. We analyzed clinical characteristics, histology, and treatment modalities. We used the Kaplan-Meier method for survival. RESULTS: 194 patients were registered; 136 patients were included. M/F ratio was 1.2, mean age 7 years old. The most frequent location was infratentorial (42.2%), supratentorial (34.9%), optic/chiasm/sellar (11%) and brainstem (11.9%). The most frequent histological types were pilocytic astrocytoma (61%), diffuse astrocytoma (10.3%), oligodendroglioma (5.2%), and other low-grade neoplasms (23.5%). Surgery was performed in 109 patients (83.2%). Chemotherapy alone was used in 17 (12.5%), while radiotherapy in 20 (14.7%). Overall survival at 5 years was 82.9% (95% CI 73.3 - 89.4). Age younger than 3 years (p=0.002), diffuse histological type (p=0.04), and location in the brainstem (p=0.001) were factors associated with a worse prognosis. CONCLUSIONS: Within the framework of the GICC, this work is one of the first steps to understand the current context of pediatric CNS tumor care in Peru. Although the reported survival rate is about the GICC goal of 60%, further improvements in care are needed to increase survival to level closer to high-resource setting and decrease long term morbidity.

Published
2022
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449. LINC-23. Factors influencing outcomes of older children with Medulloblastoma over 15 years in Peru, a resource limited setting

Author

Rosdali Diaz-Coronado, James B Reinecke, Joseph R Stanek, Jonathan L Finlay, Eddy Hernandez-Broncano, Sharon Chavez-Paredes, Yesenia Miranda-Tunque, Adela Heredia-Zelaya, Sandro Casavilca-Zambrano, Pamela Garcia-Corrochano, Luis Ojeda-Medina, Enrique Orrego-Puelles, Ebert Torres-Malca, Raymundo Sernaque-Quintana, William Quispe-Valverde, Juan Garcia-Leon, and Diana S Osorio

Subjects
Cancer Research, Oncology, Neurology (clinical)
Abstract

BACKGROUND: Medulloblastoma is the most common malignant brain tumor in children. While survival has improved in high-income countries (HIC), the outcomes for patients in low-middle-income countries (LMIC) are unclear. Therefore, we sought to determine the survival of children with Medulloblastoma at the Instituto Nacional de Enfermedades Neoplasicas (INEN) between 1997 and 2013 in Peru. METHODS: Between 1997-2013, data from 103 children older than three years with Medulloblastoma were analyzed. Fourteen patients were excluded. The patients were split into two distinct cohorts, 1997 – 2008 and 2009 – 2013, corresponding with chemotherapy regimen changes. Event-free (EFS) and overall survival (OS) were calculated using the Kaplan-Meier method, while prognostic factors were determined by univariate analysis (log-rank test). RESULTS: Eighty-nine patients were included; median age was 8.1 years (range: 3-13.9 years). The five-year OS was 62% (95% CI: 53 – 74%) while EFS was 57% (95% CI: 48 – 69%). The variables adversely affecting survival were anaplastic histology [compared to desmoplastic; OS: HR=3.4, p=0.03], metastasis [OS: HR=3.5, p=0.01; EFS: HR=4.3, p=0.004], delay in radiation therapy of 31-60 days [compared to ≤30 days; EFS: HR=2.1, p=0.04], and treatment 2009 – 2013 cohort[OS: HR=2.2, p=0.02; EFS: HR=2.0; p=0.03]. CONCLUSIONS: Outcomes for Medulloblastoma at INEN were low compared with HIC. Anaplastic sub-type, metastasis at diagnosis, delay in radiation therapy, and treatment in the period 2009 - 2013 negatively affected the outcomes in our study. Multidisciplinary teamwork, timely delivery of treatment and partnerships with loco-regional groups and colleagues in HIC is likely beneficial.

Published
2022
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