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1. Euclid preparation. Improving cosmological constraints using a new multi-tracer method with the spectroscopic and photometric samples

Author

Euclid Collaboration, Dournac, F., Blanchard, A., Ilić, S., Lamine, B., Tutusaus, I., Amara, A., Andreon, S., Auricchio, N., Aussel, H., Baldi, M., Bardelli, S., Bodendorf, C., Bonino, D., Branchini, E., Brau-Nogue, S., Brescia, M., Brinchmann, J., Camera, S., Capobianco, V., Carretero, J., Casas, S., Castellano, M., Cavuoti, S., Cimatti, A., Congedo, G., Conselice, C. J., Conversi, L., Copin, Y., Courbin, F., Courtois, H. M., Da Silva, A., Degaudenzi, H., Di Giorgio, A. M., Dinis, J., Douspis, M., Dubath, F., Dupac, X., Dusini, S., Ealet, A., Farina, M., Farrens, S., Ferriol, S., Frailis, M., Franceschi, E., Galeotta, S., Gillard, W., Gillis, B., Giocoli, C., Granett, B. R., Grazian, A., Grupp, F., Haugan, S. V. H., Holmes, W., Hook, I., Hormuth, F., Hornstrup, A., Hudelot, P., Jahnke, K., Keihänen, E., Kermiche, S., Kiessling, A., Kilbinger, M., Kubik, B., Kümmel, M., Kunz, M., Kurki-Suonio, H., Ligori, S., Lilje, P. B., Lindholm, V., Lloro, I., Maino, D., Maiorano, E., Mansutti, O., Marggraf, O., Markovic, K., Martinet, N., Marulli, F., Massey, R., Maurogordato, S., Medinaceli, E., Mei, S., Mellier, Y., Meneghetti, M., Merlin, E., Meylan, G., Moresco, M., Moscardini, L., Munari, E., Niemi, S. -M., Nightingale, J. W., Padilla, C., Paltani, S., Pasian, F., Pedersen, K., Percival, W. J., Pettorino, V., Pires, S., Polenta, G., Poncet, M., Popa, L. A., Pozzetti, L., Raison, F., Rebolo, R., Renzi, A., Rhodes, J., Riccio, G., Romelli, E., Roncarelli, M., Rossetti, E., Saglia, R., Sapone, D., Schneider, P., Secroun, A., Seidel, G., Seiffert, M., Serrano, S., Sirignano, C., Sirri, G., Stanco, L., Surace, C., Tallada-Crespí, P., Tavagnacco, D., Taylor, A. N., Tereno, I., Toledo-Moreo, R., Torradeflot, F., Valentijn, E. A., Valenziano, L., Vassallo, T., Veropalumbo, A., Wang, Y., Zacchei, A., Zamorani, G., Zoubian, J., Zucca, E., Biviano, A., Bolzonella, M., Boucaud, A., Bozzo, E., Burigana, C., Colodro-Conde, C., De Lucia, G., Di Ferdinando, D., Vigo, J. A. Escartin, Farinelli, R., Gracia-Carpio, J., Mainetti, G., Martinelli, M., Mauri, N., Neissner, C., Sakr, Z., Scottez, V., Tenti, M., Viel, M., Wiesmann, M., Akrami, Y., Allevato, V., Anselmi, S., Baccigalupi, C., Balaguera-Antolinez, A., Ballardini, M., Blot, L., Borgani, S., Bruton, S., Cabanac, R., Calabro, A., Canas-Herrera, G., Cappi, A., Carvalho, C. S., Castignani, G., Castro, T., Chambers, K. C., Contarini, S., Cooray, A. R., Coupon, J., Davini, S., De Caro, B., de la Torre, S., Desprez, G., Díaz-Sánchez, A., Di Domizio, S., Dole, H., Escoffier, S., Ferrari, A. G., Ferreira, P. G., Ferrero, I., Finelli, F., Gabarra, L., Ganga, K., García-Bellido, J., Gaztanaga, E., Giacomini, F., Gozaliasl, G., Hildebrandt, H., Munoz, A. Jimenez, Kajava, J. J. E., Kansal, V., Karagiannis, D., Kirkpatrick, C. C., Legrand, L., Libet, G., Loureiro, A., Macias-Perez, J., Maggio, G., Magliocchetti, M., Mannucci, F., Maoli, R., Martins, C. J. A. P., Matthew, S., Maurin, L., Metcalf, R. B., Migliaccio, M., Monaco, P., Moretti, C., Morgante, G., Nadathur, S., Walton, Nicholas A., Patrizii, L., Pezzotta, A., Pöntinen, M., Popa, V., Porciani, C., Potter, D., Risso, I., Rocci, P. -F., Sahlén, M., Sánchez, A. G., Schewtschenko, J. A., Schneider, A., Sefusatti, E., Sereno, M., Steinwagner, J., Tessore, N., Testera, G., Teyssier, R., Toft, S., Tosi, S., Troja, A., Tucci, M., Valiviita, J., Vergani, D., and Verza, G.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

Future data provided by the Euclid mission will allow us to better understand the cosmic history of the Universe. A metric of its performance is the figure-of-merit (FoM) of dark energy, usually estimated with Fisher forecasts. The expected FoM has previously been estimated taking into account the two main probes of Euclid, namely the three-dimensional clustering of the spectroscopic galaxy sample, and the so-called 3x2pt signal from the photometric sample (i.e., the weak lensing signal, the galaxy clustering, and their cross-correlation). So far, these two probes have been treated as independent. In this paper, we introduce a new observable given by the ratio of the (angular) two-point correlation function of galaxies from the two surveys. For identical (normalised) selection functions, this observable is unaffected by sampling noise, and its variance is solely controlled by Poisson noise. We present forecasts for Euclid where this multi-tracer method is applied and is particularly relevant because the two surveys will cover the same area of the sky. This method allows for the exploitation of the combination of the spectroscopic and photometric samples. When the correlation between this new observable and the other probes is not taken into account, a significant gain is obtained in the FoM, as well as in the constraints on other cosmological parameters. The benefit is more pronounced for a commonly investigated modified gravity model, namely the $\gamma$ parametrisation of the growth factor. However, the correlation between the different probes is found to be significant and hence the actual gain is uncertain. We present various strategies for circumventing this issue and still extract useful information from the new observable., Comment: 16 pages, 7 figures, submitted to A&A

Published
2024
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2. Euclid preparation: XLVIII. The pre-launch Science Ground Segment simulation framework

Author

Euclid Collaboration, Serrano, S., Hudelot, P., Seidel, G., Pollack, J. E., Jullo, E., Torradeflot, F., Benielli, D., Fahed, R., Auphan, T., Carretero, J., Aussel, H., Casenove, P., Castander, F. J., Davies, J. E., Fourmanoit, N., Huot, S., Kara, A., Keihänen, E., Kermiche, S., Okumura, K., Zoubian, J., Ealet, A., Boucaud, A., Bretonnière, H., Casas, R., Clément, B., Duncan, C. A. J., George, K., Kiiveri, K., Kurki-Suonio, H., Kümmel, M., Laugier, D., Mainetti, G., Mohr, J. J., Montoro, A., Neissner, C., Rosset, C., Schirmer, M., Tallada-Crespí, P., Tonello, N., Venhola, A., Verderi, A., Zacchei, A., Aghanim, N., Altieri, B., Amara, A., Andreon, S., Auricchio, N., Azzollini, R., Baccigalupi, C., Baldi, M., Bardelli, S., Basset, A., Battaglia, P., Bernardeau, F., Bodendorf, C., Bonino, D., Branchini, E., Brescia, M., Brinchmann, J., Camera, S., Candini, G. P., Capobianco, V., Carbone, C., Casas, S., Castellano, M., Castignani, G., Cavuoti, S., Cimatti, A., Cledassou, R., Colodro-Conde, C., Congedo, G., Conselice, C. J., Conversi, L., Copin, Y., Corcione, L., Courbin, F., Courtois, H. M., Crocce, M., Cropper, M., Da Silva, A., Degaudenzi, H., De Lucia, G., Di Giorgio, A. M., Dinis, J., Dubath, F., Dupac, X., Dusini, S., Farina, M., Farrens, S., Ferriol, S., Frailis, M., Franceschi, E., Franzetti, P., Galeotta, S., Garilli, B., Gillard, W., Gillis, B., Giocoli, C., Granett, B. R., Grazian, A., Grupp, F., Guzzo, L., Haugan, S. V. H., Hoar, J., Hoekstra, H., Holmes, W., Hook, I., Hormuth, F., Hornstrup, A., Jahnke, K., Joachimi, B., Kiessling, A., Kitching, T., Kohley, R., Kunz, M., Boulc'h, Q. Le, Liebing, P., Ligori, S., Lilje, P. B., Lindholm, V., Lloro, I., Maino, D., Maiorano, E., Mansutti, O., Marcin, S., Marggraf, O., Markovic, K., Martinelli, M., Martinet, N., Marulli, F., Massey, R., Maurogordato, S., Medinaceli, E., Mei, S., Melchior, M., Mellier, Y., Meneghetti, M., Merlin, E., Meylan, G., Moresco, M., Morris, P., Moscardini, L., Munari, E., Nakajima, R., Niemi, S. -M., Nutma, T., Padilla, C., Paltani, S., Pasian, F., Pedersen, K., Percival, W. J., Pettorino, V., Pires, S., Polenta, G., Poncet, M., Popa, L. A., Pozzetti, L., Raison, F., Rebolo, R., Renzi, A., Rhodes, J., Riccio, G., Romelli, E., Roncarelli, M., Rossetti, E., Rusholme, B., Saglia, R., Sakr, Z., Sánchez, A. G., Sapone, D., Sartoris, B., Sauvage, M., Schneider, P., Schrabback, T., Scodeggio, M., Secroun, A., Sirignano, C., Sirri, G., Skottfelt, J., Stanco, L., Starck, J. -L., Steinwagner, J., Taylor, A. N, Teplitz, H., Tereno, I., Toledo-Moreo, R., Tutusaus, I., Valentijn, E. A., Valenziano, L., Vassallo, T., Veropalumbo, A., Wang, Y., Weller, J., Zamorani, G., Zucca, E., Biviano, A., Bozzo, E., Di Ferdinando, D., Farinelli, R., Graciá-Carpio, J., Mauri, N., Scottez, V., Tenti, M., Akrami, Y., Allevato, V., Ballardini, M., Blanchard, A., Borgani, S., Borlaff, A. S., Bruton, S., Burigana, C., Cappi, A., Carvalho, C. S., Castro, T., Cañas-Herrera, G., Chambers, K. C., Cooray, A. R., Coupon, J., Davini, S., de la Torre, S., Desai, S., Desprez, G., Díaz-Sánchez, A., Di Domizio, S., Dole, H., Vigo, J. A. Escartin, Escoffier, S., Ferrero, I., Finelli, F., Gabarra, L., Ganga, K., Garcia-Bellido, J., Gaztanaga, E., Giacomini, F., Gozaliasl, G., Gregorio, A., Hildebrandt, H., Huertas-Company, M., Ilbert, O., Muñoz, A. Jimenez, Kajava, J. J. E., Kansal, V., Kirkpatrick, C. C., Legrand, L., Loureiro, A., Macias-Perez, J., Magliocchetti, M., Maoli, R., Martins, C. J. A. P., Matthew, S., Maurin, L., Metcalf, R. B., Migliaccio, M., Monaco, P., Morgante, G., Nadathur, S., Nucita, A. A., Pöntinen, M., Popa, V., Porciani, C., Potter, D., Reimberg, P., Schneider, A., Sereno, M., Shulevski, A., Simon, P., Mancini, A. Spurio, Stadel, J., Tewes, M., Teyssier, R., Toft, S., Tucci, M., Valiviita, J., Viel, M., and Zinchenko, I. A.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The European Space Agency's Euclid mission is one of the upcoming generation of large-scale cosmology surveys, which will map the large-scale structure in the Universe with unprecedented precision. The development and validation of the SGS pipeline requires state-of-the-art simulations with a high level of complexity and accuracy that include subtle instrumental features not accounted for previously as well as faster algorithms for the large-scale production of the expected Euclid data products. In this paper, we present the Euclid SGS simulation framework as applied in a large-scale end-to-end simulation exercise named Science Challenge 8. Our simulation pipeline enables the swift production of detailed image simulations for the construction and validation of the Euclid mission during its qualification phase and will serve as a reference throughout operations. Our end-to-end simulation framework starts with the production of a large cosmological N-body & mock galaxy catalogue simulation. We perform a selection of galaxies down to I_E=26 and 28 mag, respectively, for a Euclid Wide Survey spanning 165 deg^2 and a 1 deg^2 Euclid Deep Survey. We build realistic stellar density catalogues containing Milky Way-like stars down to H<26. Using the latest instrumental models for both the Euclid instruments and spacecraft as well as Euclid-like observing sequences, we emulate with high fidelity Euclid satellite imaging throughout the mission's lifetime. We present the SC8 data set consisting of overlapping visible and near-infrared Euclid Wide Survey and Euclid Deep Survey imaging and low-resolution spectroscopy along with ground-based. This extensive data set enables end-to-end testing of the entire ground segment data reduction and science analysis pipeline as well as the Euclid mission infrastructure, paving the way to future scientific and technical developments and enhancements., Comment: 39 pages, 25 figures, A&A submitted

Published
2024
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3. Euclid preparation. TBD. Galaxy power spectrum modelling in real space

Author

Euclid Collaboration, Pezzotta, A., Moretti, C., Zennaro, M., Dizgah, A. Moradinezhad, Crocce, M., Sefusatti, E., Ferrero, I., Pardede, K., Eggemeier, A., Barreira, A., Angulo, R. E., Marinucci, M., Quevedo, B. Camacho, de la Torre, S., Alkhanishvili, D., Biagetti, M., Breton, M. -A., Castorina, E., D'Amico, G., Desjacques, V., Guidi, M., Kärcher, M., Oddo, A., Ibanez, M. Pellejero, Porciani, C., Pugno, A., Salvalaggio, J., Sarpa, E., Veropalumbo, A., Vlah, Z., Amara, A., Andreon, S., Auricchio, N., Baldi, M., Bardelli, S., Bender, R., Bodendorf, C., Bonino, D., Branchini, E., Brescia, M., Brinchmann, J., Camera, S., Capobianco, V., Carbone, C., Cardone, V. F., Carretero, J., Casas, S., Castander, F. J., Castellano, M., Cavuoti, S., Cimatti, A., Congedo, G., Conselice, C. J., Conversi, L., Copin, Y., Corcione, L., Courbin, F., Courtois, H. M., Da Silva, A., Degaudenzi, H., Di Giorgio, A. M., Dinis, J., Dupac, X., Dusini, S., Ealet, A., Farina, M., Farrens, S., Fosalba, P., Frailis, M., Franceschi, E., Galeotta, S., Gillis, B., Giocoli, C., Granett, B. R., Grazian, A., Grupp, F., Guzzo, L., Haugan, S. V. H., Hormuth, F., Hornstrup, A., Jahnke, K., Joachimi, B., Keihänen, E., Kermiche, S., Kiessling, A., Kilbinger, M., Kitching, T., Kubik, B., Kunz, M., Kurki-Suonio, H., Ligori, S., Lilje, P. B., Lindholm, V., Lloro, I., Maiorano, E., Mansutti, O., Marggraf, O., Markovic, K., Martinet, N., Marulli, F., Massey, R., Medinaceli, E., Mellier, Y., Meneghetti, M., Merlin, E., Meylan, G., Moresco, M., Moscardini, L., Munari, E., Niemi, S. -M., Padilla, C., Paltani, S., Pasian, F., Pedersen, K., Percival, W. J., Pettorino, V., Pires, S., Polenta, G., Pollack, J. E., Poncet, M., Popa, L. A., Pozzetti, L., Raison, F., Renzi, A., Rhodes, J., Riccio, G., Romelli, E., Roncarelli, M., Rossetti, E., Saglia, R., Sapone, D., Sartoris, B., Schneider, P., Schrabback, T., Secroun, A., Seidel, G., Seiffert, M., Serrano, S., Sirignano, C., Sirri, G., Stanco, L., Surace, C., Tallada-Crespí, P., Taylor, A. N., Tereno, I., Toledo-Moreo, R., Torradeflot, F., Tutusaus, I., Valentijn, E. A., Valenziano, L., Vassallo, T., Wang, Y., Weller, J., Zamorani, G., Zoubian, J., Zucca, E., Biviano, A., Bozzo, E., Burigana, C., Colodro-Conde, C., Di Ferdinando, D., Mainetti, G., Martinelli, M., Mauri, N., Sakr, Z., Scottez, V., Tenti, M., Viel, M., Wiesmann, M., Akrami, Y., Allevato, V., Anselmi, S., Baccigalupi, C., Ballardini, M., Bernardeau, F., Blanchard, A., Borgani, S., Bruton, S., Cabanac, R., Cappi, A., Carvalho, C. S., Castignani, G., Castro, T., {n}as-Herrera, G. Ca\, Chambers, K. C., Contarini, S., Cooray, A. R., Coupon, J., Davini, S., De Lucia, G., Desprez, G., Di Domizio, S., Dole, H., Díaz-Sánchez, A., Vigo, J. A. Escartin, Escoffier, S., Ferreira, P. G., Finelli, F., Gabarra, L., Ganga, K., García-Bellido, J., Giacomini, F., Gozaliasl, G., Hall, A., Ilić, S., Joudaki, S., Kajava, J. J. E., Kansal, V., Kirkpatrick, C. C., Legrand, L., Loureiro, A., Macias-Perez, J., Magliocchetti, M., Mannucci, F., Maoli, R., Martins, C. J. A. P., Matthew, S., Maurin, L., Metcalf, R. B., Migliaccio, M., Monaco, P., Morgante, G., Nadathur, S., Walton, Nicholas A., Patrizii, L., Popa, V., Potter, D., Pourtsidou, A., Pöntinen, M., Risso, I., Rocci, P. -F., Sánchez, A. G., Sahlén, M., Schneider, A., Sereno, M., Simon, P., Mancini, A. Spurio, Steinwagner, J., Testera, G., Teyssier, R., Toft, S., Tosi, S., Troja, A., Tucci, M., Valiviita, J., Vergani, D., Verza, G., and Vielzeuf, P.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We investigate the accuracy of the perturbative galaxy bias expansion in view of the forthcoming analysis of the Euclid spectroscopic galaxy samples. We compare the performance of an Eulerian galaxy bias expansion, using state-of-art prescriptions from the effective field theory of large-scale structure (EFTofLSS), against a hybrid approach based on Lagrangian perturbation theory and high-resolution simulations. These models are benchmarked against comoving snapshots of the Flagship I N-body simulation at $z=(0.9,1.2,1.5,1.8)$, which have been populated with H$\alpha$ galaxies leading to catalogues of millions of objects within a volume of about $58\,h^{-3}\,{\rm Gpc}^3$. Our analysis suggests that both models can be used to provide a robust inference of the parameters $(h, \omega_{\rm c})$ in the redshift range under consideration, with comparable constraining power. We additionally determine the range of validity of the EFTofLSS model in terms of scale cuts and model degrees of freedom. From these tests, it emerges that the standard third-order Eulerian bias expansion can accurately describe the full shape of the real-space galaxy power spectrum up to the maximum wavenumber $k_{\rm max}=0.45\,h\,{\rm Mpc}^{-1}$, even with a measurement precision well below the percent level. In particular, this is true for a configuration with six free nuisance parameters, including local and non-local bias parameters, a matter counterterm, and a correction to the shot-noise contribution. Fixing either tidal bias parameters to physically-motivated relations still leads to unbiased cosmological constraints. We finally repeat our analysis assuming a volume that matches the expected footprint of Euclid, but without considering observational effects, as purity and completeness, showing that we can get consistent cosmological constraints over this range of scales and redshifts., Comment: 38 pages, 19 figures

Published
2023
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4. How interpersonal distance varies throughout the lifespan

Author

Ilaria Mirlisenna, Greta Bonino, Alessandro Mazza, Francesca Capiotto, Giulia Romano Cappi, Monia Cariola, Alessandro Valvo, Lucia De Francesco, and Olga Dal Monte

Subjects
Social Interaction, Interpersonal Distance, Social Behavior, Lifetime Development, Familiarity, Social Attitude, Medicine, Science
Abstract

Abstract Interpersonal Distance (IPD) is defined as the physical distance that individuals maintain between themselves and others during social interactions. While literature has extensively focused on this everyday social behavior, how IPD changes throughout the lifespan remains an open question. In this study, 864 participants, aged 3–89 years, performed the Stop Distance Paradigm in their real-life environments, and we measured the distance they kept from both familiar and unfamiliar others during social interactions. We found that IPD not only differs based on the identity of the other person (familiar versus unfamiliar) but critically declines as a function of age, following two distinct non-linear trends for familiar and unfamiliar others. Moreover, behavioral variability also undergoes a lifetime development, with IPD becoming more stable as age increases. Overall, the present study suggests that IPD is a complex and acquired behavior that changes throughout the lifespan and varies according to individual and situational variables.

Published
2024
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7. Rare de novo damaging DNA variants are enriched in attention-deficit/hyperactivity disorder and implicate risk genes

Author

Emily Olfson, Luis C. Farhat, Wenzhong Liu, Lawrence A. Vitulano, Gwyneth Zai, Monicke O. Lima, Justin Parent, Guilherme V. Polanczyk, Carolina Cappi, James L. Kennedy, and Thomas V. Fernandez

Subjects
Science
Abstract

Abstract Research demonstrates the important role of genetic factors in attention-deficit/hyperactivity disorder (ADHD). DNA sequencing of families provides a powerful approach for identifying de novo (spontaneous) variants, leading to the discovery of hundreds of clinically informative risk genes for other childhood neurodevelopmental disorders. This approach has yet to be extensively leveraged in ADHD. We conduct whole-exome DNA sequencing in 152 families, comprising a child with ADHD and both biological parents, and demonstrate a significant enrichment of rare and ultra-rare de novo gene-damaging mutations in ADHD cases compared to unaffected controls. Combining these results with a large independent case-control DNA sequencing cohort (3206 ADHD cases and 5002 controls), we identify lysine demethylase 5B (KDM5B) as a high-confidence risk gene for ADHD and estimate that 1057 genes contribute to ADHD risk. Using our list of genes harboring ultra-rare de novo damaging variants, we show that these genes overlap with previously reported risk genes for other neuropsychiatric conditions and are enriched in several canonical biological pathways, suggesting early neurodevelopmental underpinnings of ADHD. This work provides insight into the biology of ADHD and demonstrates the discovery potential of DNA sequencing in larger parent-child trio cohorts.

Published
2024
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9. An evolutionary perspective on complex neuropsychiatric disease

Author

McClellan, Jon M., Zoghbi, Anthony W., Buxbaum, Joseph D., Cappi, Carolina, Crowley, James J., Flint, Jonathan, Grice, Dorothy E., Gulsuner, Suleyman, Iyegbe, Conrad, Jain, Sanjeev, Kuo, Po-Hsiu, Lattig, Maria Claudia, Passos-Bueno, Maria Rita, Purushottam, Meera, Stein, Dan J., Sunshine, Anna B., Susser, Ezra S., Walsh, Christopher A., Wootton, Olivia, and King, Mary-Claire

Published
2024
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12. The Athena X-ray Integral Field Unit: a consolidated design for the system requirement review of the preliminary definition phase

Author

Barret, Didier, Albouys, Vincent, Herder, Jan-Willem den, Piro, Luigi, Cappi, Massimo, Huovelin, Juhani, Kelley, Richard, Mas-Hesse, J. Miguel, Paltani, Stéphane, Rauw, Gregor, Rozanska, Agata, Svoboda, Jiri, Wilms, Joern, Yamasaki, Noriko, Audard, Marc, Bandler, Simon, Barbera, Marco, Barcons, Xavier, Bozzo, Enrico, Ceballos, Maria Teresa, Charles, Ivan, Costantini, Elisa, Dauser, Thomas, Decourchelle, Anne, Duband, Lionel, Duval, Jean-Marc, Fiore, Fabrizio, Gatti, Flavio, Goldwurm, Andrea, Hartog, Roland den, Jackson, Brian, Jonker, Peter, Kilbourne, Caroline, Korpela, Seppo, Macculi, Claudio, Mendez, Mariano, Mitsuda, Kazuhisa, Molendi, Silvano, Pajot, François, Pointecouteau, Etienne, Porter, Frederick, Pratt, Gabriel W., Prêle, Damien, Ravera, Laurent, Sato, Kosuke, Schaye, Joop, Shinozaki, Keisuke, Skup, Konrad, Soucek, Jan, Thibert, Tanguy, Vink, Jacco, Webb, Natalie, Chaoul, Laurence, Raulin, Desi, Simionescu, Aurora, Torrejon, Jose Miguel, Acero, Fabio, Branduardi-Raymont, Graziella, Ettori, Stefano, Finoguenov, Alexis, Grosso, Nicolas, Kaastra, Jelle, Mazzotta, Pasquale, Miller, Jon, Miniutti, Giovanni, Nicastro, Fabrizio, Sciortino, Salvatore, Yamaguchi, Hiroya, Beaumont, Sophie, Cucchetti, Edoardo, D’Andrea, Matteo, Eckart, Megan, Ferrando, Philippe, Kammoun, Elias, Lotti, Simone, Mesnager, Jean-Michel, Natalucci, Lorenzo, Peille, Philippe, de Plaa, Jelle, Ardellier, Florence, Argan, Andrea, Bellouard, Elise, Carron, Jérôme, Cavazzuti, Elisabetta, Fiorini, Mauro, Khosropanah, Pourya, Martin, Sylvain, Perry, James, Pinsard, Frederic, Pradines, Alice, Rigano, Manuela, Roelfsema, Peter, Schwander, Denis, Torrioli, Guido, Ullom, Joel, Vera, Isabel, Villegas, Eduardo Medinaceli, Zuchniak, Monika, Brachet, Frank, Cicero, Ugo Lo, Doriese, William, Durkin, Malcom, Fioretti, Valentina, Geoffray, Hervé, Jacques, Lionel, Kirsch, Christian, Smith, Stephen, Adams, Joseph, Gloaguen, Emilie, Hoogeveen, Ruud, van der Hulst, Paul, Kiviranta, Mikko, van der Kuur, Jan, Ledot, Aurélien, van Leeuwen, Bert-Joost, van Loon, Dennis, Lyautey, Bertrand, Parot, Yann, Sakai, Kazuhiro, van Weers, Henk, Abdoelkariem, Shariefa, Adam, Thomas, Adami, Christophe, Aicardi, Corinne, Akamatsu, Hiroki, Alonso, Pablo Eleazar Merino, Amato, Roberta, André, Jérôme, Angelinelli, Matteo, Anon-Cancela, Manuel, Anvar, Shebli, Atienza, Ricardo, Attard, Anthony, Auricchio, Natalia, Balado, Ana, Bancel, Florian, Barusso, Lorenzo Ferrari, Bascuñan, Arturo, Bernard, Vivian, Berrocal, Alicia, Blin, Sylvie, Bonino, Donata, Bonnet, François, Bonny, Patrick, Boorman, Peter, Boreux, Charles, Bounab, Ayoub, Boutelier, Martin, Boyce, Kevin, Brienza, Daniele, Bruijn, Marcel, Bulgarelli, Andrea, Calarco, Simona, Callanan, Paul, Campello, Alberto Prada, Camus, Thierry, Canourgues, Florent, Capobianco, Vito, Cardiel, Nicolas, Castellani, Florent, Cheatom, Oscar, Chervenak, James, Chiarello, Fabio, Clerc, Laurent, Clerc, Nicolas, Cobo, Beatriz, Coeur-Joly, Odile, Coleiro, Alexis, Colonges, Stéphane, Corcione, Leonardo, Coriat, Mickael, Coynel, Alexandre, Cuttaia, Francesco, D’Ai, Antonino, D’anca, Fabio, Dadina, Mauro, Daniel, Christophe, Dauner, Lea, DeNigris, Natalie, Dercksen, Johannes, DiPirro, Michael, Doumayrou, Eric, Dubbeldam, Luc, Dupieux, Michel, Dupourqué, Simon, Durand, Jean Louis, Eckert, Dominique, Eiriz, Valvanera, Ercolani, Eric, Etcheverry, Christophe, Finkbeiner, Fred, Fiocchi, Mariateresa, Fossecave, Hervé, Franssen, Philippe, Frericks, Martin, Gabici, Stefano, Gant, Florent, Gao, Jian-Rong, Gastaldello, Fabio, Genolet, Ludovic, Ghizzardi, Simona, Gil, Ma Angeles Alcacera, Giovannini, Elisa, Godet, Olivier, Gomez-Elvira, Javier, Gonzalez, Raoul, Gonzalez, Manuel, Gottardi, Luciano, Granat, Dolorès, Gros, Michel, Guignard, Nicolas, Hieltjes, Paul, Hurtado, Adolfo Jesús, Irwin, Kent, Jacquey, Christian, Janiuk, Agnieszka, Jaubert, Jean, Jiménez, Maria, Jolly, Antoine, Jourdan, Thierry, Julien, Sabine, Kedziora, Bartosz, Korb, Andrew, Kreykenbohm, Ingo, König, Ole, Langer, Mathieu, Laudet, Philippe, Laurent, Philippe, Laurenza, Monica, Lesrel, Jean, Ligori, Sebastiano, Lorenz, Maximilian, Luminari, Alfredo, Maffei, Bruno, Maisonnave, Océane, Marelli, Lorenzo, Massonet, Didier, Maussang, Irwin, Melchor, Alejandro Gonzalo, Le Mer, Isabelle, Millan, Francisco Javier San, Millerioux, Jean-Pierre, Mineo, Teresa, Minervini, Gabriele, Molin, Alexeï, Monestes, David, Montinaro, Nicola, Mot, Baptiste, Murat, David, Nagayoshi, Kenichiro, Nazé, Yaël, Noguès, Loïc, Pailot, Damien, Panessa, Francesca, Parodi, Luigi, Petit, Pascal, Piconcelli, Enrico, Pinto, Ciro, Plaza, Jose Miguel Encinas, Plaza, Borja, Poyatos, David, Prouvé, Thomas, Ptak, Andy, Puccetti, Simonetta, Puccio, Elena, Ramon, Pascale, Reina, Manuel, Rioland, Guillaume, Rodriguez, Louis, Roig, Anton, Rollet, Bertrand, Roncarelli, Mauro, Roudil, Gilles, Rudnicki, Tomasz, Sanisidro, Julien, Sciortino, Luisa, Silva, Vitor, Sordet, Michael, Soto-Aguilar, Javier, Spizzi, Pierre, Surace, Christian, Sánchez, Miguel Fernández, Taralli, Emanuele, Terrasa, Guilhem, Terrier, Régis, Todaro, Michela, Ubertini, Pietro, Uslenghi, Michela, de Vaate, Jan Geralt Bij, Vaccaro, Davide, Varisco, Salvatore, Varnière, Peggy, Vibert, Laurent, Vidriales, María, Villa, Fabrizio, Vodopivec, Boris Martin, Volpe, Angela, de Vries, Cor, Wakeham, Nicholas, Walmsley, Gavin, Wise, Michael, de Wit, Martin, and Woźniak, Grzegorz

Published
2023
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13. Coabitare il Territorio: il Turismo Responsabile come Pratica di Ospitalità e Cura delle Comunità

Author

Pierluigi Musarò, Valentina Cappi, and Marta Vignola

Subjects
tourism, sustainability, responsible tourism, festival IT.A.CÀ, sustainable tourism, Human ecology. Anthropogeography, GF1-900
Abstract

Lo studio del turismo è una delle porte d’ingresso privilegiate per comprendere il territorio, non solo dal punto di vista economico. Il turismo svolge un ruolo essenziale nella dialettica sociale e spaziale che assegna significato ai luoghi: da una parte alimenta l’immaginario individuale e collettivo attraverso la produzione d’icone e di rappresentazioni; dall’altra modella i luoghi, che si fanno “turistici” attraverso trasformazioni visibili che spazializzano quelle stesse immagini. Dagli anni Settanta del secolo scorso, diversi osservatori hanno denunciato il fenomeno turistico come una nuova forma di alienazione, distruzione dell’ambiente o imperialismo. Sulla scia di questi ed altri richiami alla necessità di ripensare e governare un settore in continua crescita, è nato il cosiddetto turismo responsabile, una modalità di viaggio che soddisfa e rispetta i bisogni dei viaggiatori e delle regioni ospitanti e allo stesso tempo protegge e migliora le opportunità di determinati territori. Partendo da una riflessione sulle dimensioni, gli impatti e i cambiamenti in atto di uno dei fenomeni caratterizzanti la contemporaneità, questo articolo, così come la special issue che esso introduce, prende come caso di studio IT.A.CÀ_migranti e viaggiatori, il primo festival a livello europeo focalizzato esplicitamente sul tema del turismo responsabile. Il viaggio nelle diverse edizioni di IT.A.CÀ_migranti e viaggiatori permette di valutare presupposti, esiti e potenzialità future di esperienze e pratiche che negli ultimi anni, attraverso processi partecipativi di condivisione, co-progettazione, dialogo e sperimentazione, hanno cercato di coniugare la sostenibilità del turismo con il benessere dei cittadini, immaginando una valorizzazione del territorio che promuova la transizione verso una coabitazione sostenibile della Terra.

Published
2024
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14. NIKA2 observations of 3 low-mass galaxy clusters at z ~ 1: Pressure profile and YSZ – M relation

Author

Adam R., Ricci M., Eckert D., Ade P., Ajeddig H., Altieri B., André P., Artis E., Aussel H., Beelen A., Benoist C., Benoît A., Berta S., Bing L., Birkinshaw M., Bourrion O., Boutigny D., Bremer M., Calvo M., Cappi A., Catalano A., De Petris M., Désert F.-X., Doyle S., Driessen E.F.C., Faccioli L., Ferrari C., Gastaldello F., Giles P., Gomez A., Goupy J., Hahn O., Hanser C., Horellou C., Kéruzoré F., Koulouridis E., Kramer C., Ladjelate B., Lagache G., Leclercq S., Lestrade J.-F., Macías-Pérez J.F., Madden S., Maughan B., Maurogordato S., Maury A., Mauskopf P., Monfardini A., Muñoz-Echeverría M., Pacaud F., Perotto L., Pierre M., Pisano G., Pompei E., Ponthieu N., Revéret V., Rigby A., Ritacco A., Romero C., Roussel H., Ruppin F., Sereno M., Schuster K., Sievers A., Vidal G. Tintoré, Tucker C., and Zylka R.

Subjects
Physics, QC1-999
Abstract

Three galaxy clusters selected from the XXL X-ray survey at high redshift and low mass (z ~ 1 and M500 ~ 1 – 2 × 1014 M⊙) were observed with NIKA2 to image their Sunyaev-Zel'dovich effect (SZ) signal. They all present an SZ morphology, together with the comparison with X-ray and optical data, that indicates dynamical activity related to merging events. Despite their disturbed intracluster medium, their high redshifts, and their low masses, the three clusters follow remarkably well the pressure profile and the SZ flux-mass relation expected from standard evolution. This suggests that the physics that drives cluster formation is already in place at z ~ 1 down to M500 ~ 1014 M⊙.

Published
2024
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16. The thalamus and its subnuclei—a gateway to obsessive-compulsive disorder

Author

Weeland, Cees J., Kasprzak, Selina, de Joode, Niels T., Abe, Yoshinari, Alonso, Pino, Ameis, Stephanie H., Anticevic, Alan, Arnold, Paul D., Balachander, Srinivas, Banaj, Nerisa, Bargallo, Nuria, Batistuzzo, Marcelo C., Benedetti, Francesco, Beucke, Jan C., Bollettini, Irene, Brecke, Vilde, Brem, Silvia, Cappi, Carolina, Cheng, Yuqi, Cho, Kang Ik K., Costa, Daniel L. C., Dallaspezia, Sara, Denys, Damiaan, Eng, Goi Khia, Ferreira, Sónia, Feusner, Jamie D., Fontaine, Martine, Fouche, Jean-Paul, Grazioplene, Rachael G., Gruner, Patricia, He, Mengxin, Hirano, Yoshiyuki, Hoexter, Marcelo Q., Huyser, Chaim, Hu, Hao, Jaspers-Fayer, Fern, Kathmann, Norbert, Kaufmann, Christian, Kim, Minah, Koch, Kathrin, Bin Kwak, Yoo, Kwon, Jun Soo, Lazaro, Luisa, Li, Chiang-shan R., Lochner, Christine, Marsh, Rachel, Martínez-Zalacaín, Ignacio, Mataix-Cols, David, Menchón, Jose M., Minnuzi, Luciano, Moreira, Pedro Silva, Morgado, Pedro, Nakagawa, Akiko, Nakamae, Takashi, Narayanaswamy, Janardhanan C., Nurmi, Erika L., Ortiz, Ana E., Pariente, Jose C., Piacentini, John, Picó-Pérez, Maria, Piras, Fabrizio, Piras, Federica, Pittenger, Christopher, Reddy, Y. C. Janardhan, Rodriguez-Manrique, Daniela, Sakai, Yuki, Shimizu, Eiji, Shivakumar, Venkataram, Simpson, Helen Blair, Soreni, Noam, Soriano-Mas, Carles, Sousa, Nuno, Spalletta, Gianfranco, Stern, Emily R., Stevens, Michael C., Stewart, S. Evelyn, Szeszko, Philip R., Takahashi, Jumpei, Tanamatis, Tais, Tang, Jinsong, Thorsen, Anders Lillevik, Tolin, David, van der Werf, Ysbrand D., van Marle, Hein, van Wingen, Guido A., Vecchio, Daniela, Venkatasubramanian, G., Walitza, Susanne, Wang, Jicai, Wang, Zhen, Watanabe, Anri, Wolters, Lidewij H., Xu, Xiufeng, Yun, Je-Yeon, Zhao, Qing, White, Tonya, Thompson, Paul M., Stein, Dan J., van den Heuvel, Odile A., and Vriend, Chris

Published
2022
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17. Cellular and Extracellular White Matter Abnormalities in Obsessive-Compulsive Disorder: A Diffusion Magnetic Resonance Imaging Study

Author

Maziero, Maria Paula, Seitz-Holland, Johanna, Cho, Kang Ik K., Goldenberg, Joshua E., Tanamatis, Taís W., Diniz, Juliana B., Cappi, Carolina, Alice de Mathis, Maria, Otaduy, Maria C.G., da Graça Morais Martin, Maria, de Melo Felipe da Silva, Renata, Shavitt, Roseli G., Batistuzzo, Marcelo C., Lopes, Antonio C., Miguel, Eurípedes C., Pasternak, Ofer, and Hoexter, Marcelo Q.

Published
2021
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18. The VIMOS Public Extragalactic Redshift Survey (VIPERS): Galaxy segregation inside filaments at $z \simeq 0.7$

Author

Malavasi, N., Arnouts, S., Vibert, D., de la Torre, S., Moutard, T., Pichon, C., Davidzon, I., Kraljic, K., Bolzonella, M., Guzzo, L., Garilli, B., Scodeggio, M., Granett, B. R., Abbas, U., Adami, C., Bottini, D., Cappi, A., Cucciati, O., Franzetti, P., Fritz, A., Iovino, A., Krywult, J., Brun, V. Le, Fèvre, O. Le, Maccagni, D., Małek, K., Marulli, F., Polletta, M., Pollo, A., Tasca, L., Tojeiro, R., Vergani, D., Zanichelli, A., Bel, J., Branchini, E., Coupon, J., De Lucia, G., Dubois, Y., Hawken, A., Ilbert, O., Laigle, C., Moscardini, L., Sousbie, T., Treyer, M., and Zamorani, G.

Subjects
Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We present the first quantitative detection of large-scale filamentary structure at $z \simeq 0.7$ in the large cosmological volume probed by the VIMOS Public Extragalactic Redshift Survey (VIPERS). We use simulations to show the capability of VIPERS to recover robust topological features in the galaxy distribution, in particular the filamentary network. We then investigate how galaxies with different stellar masses and stellar activities are distributed around the filaments and find a significant segregation, with the most massive or quiescent galaxies being closer to the filament axis than less massive or active galaxies. The signal persists even after down-weighting the contribution of peak regions. Our results suggest that massive and quiescent galaxies assemble their stellar mass through successive mergers during their migration along filaments towards the nodes of the cosmic web. On the other hand, low-mass star-forming galaxies prefer the outer edge of filaments, a vorticity rich region dominated by smooth accretion, as predicted by the recent spin alignment theory. This emphasizes the role of large scale cosmic flows in shaping galaxy properties., Comment: 7 pages, 3 figures, accepted for publication in MNRAS

Published
2016
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20. The high energy Universe at ultra-high resolution: the power and promise of X-ray interferometry

Author

Uttley, Phil, Hartog, Roland den, Bambi, Cosimo, Barret, Didier, Bianchi, Stefano, Bursa, Michal, Cappi, Massimo, Casella, Piergiorgio, Cash, Webster, Costantini, Elisa, Dauser, Thomas, Trigo, Maria Diaz, Gendreau, Keith, Grinberg, Victoria, Herder, Jan-Willem den, Ingram, Adam, Kara, Erin, Markoff, Sera, Mingo, Beatriz, Panessa, Francesca, Poppenhäger, Katja, Różańska, Agata, Svoboda, Jiri, Wijers, Ralph, Willingale, Richard, Wilms, Jörn, and Wise, Michael

Published
2021
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21. Latin American Trans‐ancestry INitiative for OCD genomics (LATINO): Study protocol.

Author

Crowley, James J., Cappi, Carolina, Ochoa‐Panaifo, Marcos E., Frederick, Renee M., Kook, Minjee, Wiese, Andrew D., Rancourt, Diana, Atkinson, Elizabeth G., Giusti‐Rodriguez, Paola, Anderberg, Jacey L., Abramowitz, Jonathan S, Adorno, Victor R, Aguirre, Cinthia, Alves, Gilberto S, Alves, Gustavo S, Ancalade, NaEshia, Anderberg, Jacey L, Arellano Espinosa, Alejandro A, Arnold, Paul D, and Atkinson, Elizabeth G

Published
2024
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22. De Novo Damaging DNA Coding Mutations Are Associated With Obsessive-Compulsive Disorder and Overlap With Tourette’s Disorder and Autism

Author

Cappi, Carolina, Oliphant, Melody E., Péter, Zsanett, Zai, Gwyneth, Conceição do Rosário, Maria, Sullivan, Catherine A.W., Gupta, Abha R., Hoffman, Ellen J., Virdee, Manmeet, Olfson, Emily, Abdallah, Sarah B., Willsey, A. Jeremy, Shavitt, Roseli G., Miguel, Euripedes C., Kennedy, James L., Richter, Margaret A., and Fernandez, Thomas V.

Published
2020
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23. Trends in clinical profiles, organ support use and outcomes of patients with cancer requiring unplanned ICU admission: a multicenter cohort study

Author

Zampieri, Fernando G., Romano, Thiago G., Salluh, Jorge I. F., Taniguchi, Leandro U., Mendes, Pedro V., Nassar, Jr, Antonio P., Costa, Roberto, Viana, William N., Maia, Marcelo O., Lima, Mariza F. A., Cappi, Sylas B., Carvalho, Alexandre G. R., De Marco, Fernando V. C., Santino, Marcelo S., Perecmanis, Eric, Miranda, Fabio G., Ramos, Grazielle V., Silva, Aline R., Hoff, Paulo M., Bozza, Fernando A., and Soares, Marcio

Published
2021
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24. A fast and long-lived outflow from the supermassive black hole in NGC 5548

Author

Kaastra, J. S., Kriss, G. A., Cappi, M., Mehdipour, M., Petrucci, P. -O., Steenbrugge, K. C., Arav, N., Behar, E., Bianchi, S., Boissay, R., Branduardi-Raymont, G., Chamberlain, C., Costantini, E., Ely, J. C., Ebrero, J., Di Gesu, L., Harrison, F. A., Kaspi, S., Malzac, J., De Marco, B., Matt, G., Nandra, K., Paltani, S., Person, R., Peterson, B. M., Pinto, C., Ponti, G., Nuñez, F. Pozo, De Rosa, A., Seta, H., Ursini, F., de Vries, C. P., Walton, D. J., and Whewell, M.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract

Supermassive black holes in the nuclei of active galaxies expel large amounts of matter through powerful winds of ionized gas. The archetypal active galaxy NGC 5548 has been studied for decades, and high-resolution X-ray and UV observations have previously shown a persistent ionized outflow. An observing campaign in 2013 with six space observatories shows the nucleus to be obscured by a long-lasting, clumpy stream of ionized gas never seen before. It blocks 90% of the soft X-ray emission and causes simultaneous deep, broad UV absorption troughs. The outflow velocities of this gas are up to five times faster than those in the persistent outflow, and at a distance of only a few light days from the nucleus, it may likely originate from the accretion disk., Comment: 25 pages, 8 figures. This is the author's version of the work. It is posted here by permission of the AAAS for personal use, not for redistribution. The definitive version was published in Science, electronically available at Science Express (June 19, 2014). For a brief video explaining the key results of this paper, please visit http://www.issibern.ch/teams/ngc5548/?page_id=25

Published
2014
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25. The VIMOS Public Extragalactic Redshift Survey (VIPERS): $\Omega_{\rm m_0}$ from the galaxy clustering ratio measured at $z \sim 1$

Author

Bel, J., Marinoni, C., Granett, B. R., Guzzo, L., Peacock, J. A., Branchini, E., Cucciati, O., de la Torre, S., Iovino, A., Percival, W. J., Steigerwald, H., Abbas, U., Adami, C., Arnouts, S., Bolzonella, M., Bottini, D., Cappi, A., Coupon, J., Davidzon, I., De Lucia, G., Fritz, A., Franzetti, P., Fumana, M., Garilli, B., Ilbert, O., Krywult, J., Brun, V. Le, Fèvre, O. Le, Maccagni, D., Małek, K., Marulli, F., McCracken, H. J., Paioro, L., Polletta, M., Pollo, A., Schlagenhaufer, H., Scodeggio, M., Tasca, L. A. M., Tojeiro, R., Vergani, D., Zanichelli, A., Burden, A., Di Porto, C., Marchetti, A., Mellier, Y., Moscardini, L., Nichol, R. C., Phleps, S., Wolk, M., and Zamorani, G.

Subjects
Astrophysics - Cosmology and Extragalactic Astrophysics
Abstract

We use a sample of about 22,000 galaxies at $0.65

Published
2013
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26. The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35016 galaxies and AGN out to z~6.7 selected with 17.5<=i_{AB}<=24.7

Author

Fevre, O. Le, Cassata, P., Cucciati, O., Garilli, B., Ilbert, O., Brun, V. Le, Maccagni, D., Moreau, C., Scodeggio, M., Tresse, L., Zamorani, G., Adami, C., Arnouts, S., Bardelli, S., Bolzonella, M., Bondi, M., Bongiorno, A., Bottini, D., Cappi, A., Charlot, S., Ciliegi, P., Contini, T., de la Torre, S., Foucaud, S., Franzetti, P., Gavignaud, I., Guzzo, L., Iovino, A., Lemaux, B., McCracken, H. J., Marano, B., Marinoni, C., Mazure, A., Mellier, Y., Merighi, R., Merluzzi, P., Paltani, S., Pello, R., Pollo, A., Pozzetti, L., Scaramella, R., Vergani, D., Vettolani, G., Zanichelli, A., and Zucca, E.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We describe the completed VIMOS VLT Deep Survey, and the final data release of 35016 galaxies and type-I AGN with measured spectroscopic redshifts up to redshift z~6.7, in areas 0.142 to 8.7 square degrees, and volumes from 0.5x10^6 to 2x10^7h^-3Mpc^3. We have selected samples of galaxies based solely on their i-band magnitude reaching i_{AB}=24.75. Spectra have been obtained with VIMOS on the ESO-VLT, integrating 0.75h, 4.5h and 18h for the Wide, Deep, and Ultra-Deep nested surveys. A total of 1263 galaxies have been re-observed independently within the VVDS, and from the VIPERS and MASSIV surveys. They are used to establish the redshift measurements reliability, to assess completeness, and to provide a weighting scheme taking into account the survey selection function. We describe the main properties of the VVDS samples, and the VVDS is compared to other spectroscopic surveys. In total we have obtained spectroscopic redshifts for 34594 galaxies, 422 type-I AGN, and 12430 Galactic stars. The survey has enabled to identify galaxies up to very high redshifts with 4669 redshifts in 1<=z_{spec}<=2, 561 in 2<=z_{spec}<=3 and 468 with z_{spec}>3, and specific populations like LAE have been identified out to z=6.62. We show that the VVDS occupies a unique place in the parameter space defined by area, depth, redshift coverage, and number of spectra. The VVDS provides a comprehensive survey of the distant universe, covering all epochs since z, or more than 12 Gyr of cosmic time, with a uniform selection, the largest such sample to date. A wealth of science results derived from the VVDS have shed new light on the evolution of galaxies and AGN, and their distribution in space, over this large cosmic time. A final public release of the complete VVDS spectroscopic redshift sample is available at http://cesam.lam.fr/vvds., Comment: Submitted 30 June 2013, Accepted 22 August 2013. Updated with published version

Published
2013
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27. The VIMOS Public Extragalactic Redshift Survey (VIPERS): spectral classification through Principal Component Analysis

Author

Marchetti, A., Granett, B. R., Guzzo, L., Fritz, A., Garilli, B., Scodeggio, M., Abbas, U., Adami, C., Arnouts, S., Bolzonella, M., Bottini, D., Cappi, A., Coupon, J., Cucciati, O., De Lucia, G., de la Torre, S., Franzetti, P., Fumana, M., Ilbert, O., Iovino, A., Krywult, J., Brun, V. Le, Fevre, O. Le, Maccagni, D., Malek, K., Marulli, F., McCracken, H. J., Meneux, B., Paioro, L., Polletta, M., Pollo, A., Schlagenhaufer, H., Tasca, L., Tojeiro, R., Vergani, D., Zanichelli, A., Bel, J., Bersanelli, M., Blaizot, J., Branchini, E., Burden, A., Davidzon, I., Di Porto, C., Guennou, L., Marinoni, C., Mellier, Y., Moscardini, L., Nichol, R. C., Peacock, J. A., Percival, W. J., Phleps, S., Schimd, C., Wolk, M., and Zamorani, G.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We develop a Principal Component Analysis aimed at classifying a sub-set of 27,350 spectra of galaxies in the range 0.4 < z < 1.0 collected by the VIMOS Public Extragalactic Redshift Survey (VIPERS). We apply an iterative algorithm to simultaneously repair parts of spectra affected by noise and/or sky residuals, and reconstruct gaps due to rest-frame transformation, and obtain a set of orthogonal spectral templates that span the diversity of galaxy types. By taking the three most significant components, we find that we can describe the whole sample without contamination from noise. We produce a catalogue of eigen-coefficients and template spectra that will be part of future VIPERS data releases. Our templates effectively condense the spectral information into two coefficients that can be related to the age and star formation rate of the galaxies. We examine the spectrophotometric types in this space and identify early, intermediate, late and starburst galaxies., Comment: 15 pages, 20 images, accepted for publication in MNRAS: MN-12-1739-MJ.R1

Published
2012
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28. Understanding the shape of the galaxy two-point correlation function at z~1 in the COSMOS field

Author

de la Torre, S., Guzzo, L., Kovac, K., Porciani, C., Abbas, U., Meneux, B., Carollo, C. M., Contini, T., Kneib, J. -P., Fevre, O. Le, Lilly, S. J., Mainieri, V., Renzini, A., Sanders, D., Scodeggio, M., Scoville, N., Zamorani, G., Bardelli, S., Bolzonella, M., Bongiorno, A., Caputi, K., Coppa, G., Cucciati, O., de Ravel, L., Franzetti, P., Garilli, B., Iovino, A., Kampczyk, P., Knobel, C., Koekemoer, A. M., Lamareille, F., Borgne, J. -F. Le, Brun, V. Le, Maier, C., Mignoli, M., Pello, R., Peng, Y., Perez-Montero, E., Ricciardelli, E., Silverman, J., Tanaka, M., Tasca, L., Tresse, L., Vergani, D., Welikala, N., Zucca, E., Bottini, D., Cappi, A., Cassata, P., Cimatti, A., Fumana, M., Ilbert, O., Leauthaud, A., Maccagni, D., Marinoni, C., McCracken, H. J., Memeo, P., Nair, P., Oesch, P., Pozzetti, L., Presotto, V., and Scaramella, R.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We investigate how the shape of the galaxy two-point correlation function as measured in the zCOSMOS survey depends on local environment, quantified in terms of the density contrast on scales of 5 Mpc/h. We show that the flat shape previously observed at redshifts between z=0.6 and z=1 can be explained by this volume being simply 10% over-abundant in high-density environments, with respect to a Universal density probability distribution function. When galaxies corresponding to the top 10% tail of the distribution are excluded, the measured w_p(r_p) steepens and becomes indistinguishable from LCDM predictions on all scales. This is the same effect recognised by Abbas & Sheth in the SDSS data at z~0 and explained as a natural consequence of halo-environment correlations in a hierarchical scenario. Galaxies living in high-density regions trace dark matter halos with typically higher masses, which are more correlated. If the density probability distribution function of the sample is particularly rich in high-density regions because of the variance introduced by its finite size, this produces a distorted two-point correlation function. We argue that this is the dominant effect responsible for the observed "peculiar" clustering in the COSMOS field., Comment: 6 pages, 3 figures, accepted for publication in MNRAS

Published
2010
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29. The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z~1

Author

de la Torre, S., Fèvre, O. Le, Porciani, C., Guzzo, L., Meneux, B., Abbas, U., Tasca, L., Carollo, C. M., Contini, T., Kneib, J. -P., Lilly, S. J., Mainieri, V., Renzini, A., Scodeggio, M., Zamorani, G., Bardelli, S., Bolzonella, M., Bongiorno, A., Caputi, K., Coppa, G., Cucciati, O., de Ravel, L., Franzetti, P., Garilli, B., Halliday, C., Iovino, A., Kampczyk, P., Knobel, C., Koekemoer, A. M., Kovac, K., Lamareille, F., Borgne, J. -F. Le, Brun, V. Le, Maier, C., Mignoli, M., Pelló, R., Peng, Y., Perez-Montero, E., Ricciardelli, E., Silverman, J., Tanaka, M., Tresse, L., Vergani, D., Zucca, E., Bottini, D., Cappi, A., Cassata, P., Cimatti, A., Leauthaud, A., Maccagni, D., Marinoni, C., McCracken, H. J., Memeo, P., Oesch, P., Pozzetti, L., and Scaramella, R.

Subjects
Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We measure the spatial clustering of galaxies as a function of their morphological type at z~0.8, for the first time in a deep redshift survey with full morphological information. This is obtained by combining high-resolution HST imaging and VLT spectroscopy for about 8,500 galaxies to I_AB=22.5 with accurate spectroscopic redshifts from the zCOSMOS-Bright redshift survey. At this epoch, early-type galaxies already show a significantly stronger clustering than late-type galaxies on all probed scales. A comparison to the SDSS at z~0.1, shows that the relative clustering strength between early and late morphological classes tends to increase with cosmic time at small separations, while on large scales it shows no significant evolution since z~0.8. This suggests that most early-type galaxies had already formed in intermediate and dense environments at this epoch. Our results are consistent with a picture in which the relative clustering of different morphological types between z~1 and z~0, reflects the evolving role of environment in the morphological transformation of galaxies, on top of the global mass-driven evolution., Comment: 10 pages, 10 figures, accepted for publication in MNRAS

Published
2009
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30. Autonomic and hedonic response to affective touch in autism spectrum disorder.

Author

Capiotto, Francesca, Romano Cappi, Giulia, Mirlisenna, Ilaria, Mazza, Alessandro, Cicinelli, Giovanni, Lauritano, Chiara, Keller, Roberto, and Dal Monte, Olga

Abstract

Interpersonal touch plays a crucial role in shaping relationships and encouraging social connections. Failure in processing tactile input or abnormal tactile sensitivity may hamper social behaviors and have severe consequences in individuals' relational lives. Autism Spectrum Disorder (ASD) is characterized by both sensory disruptions and social impairments, making affective touch an ideal meeting point for understanding these features in ASD individuals. By integrating behavioral and physiological measures, we investigated the effects of affective touch on adult individuals with ASD from both an implicit and explicit perspective. Specifically, at an implicit level, we investigated whether and how receiving an affective touch influenced participants' skin conductance tonic and phasic components. At the explicit level, we delved into the affective and unpleasant features of affective touch. Overall, we observed lower skin conductance level in ASD compared to TD subjects. Interestingly, the typically developing (TD) group showed an increased autonomic response for affective touch compared to a control touch, while ASD subjects' autonomic response did not differ between the two conditions. Furthermore, ASD participants provided higher ratings for both the affective and unpleasant components of the touch, compared to TD subjects. Our results reveal a noteworthy discrepancy in ASD population between the subjective experience, characterized by amplified hedonic but also unpleasant responses, and the physiological response, marked by a lack of autonomic activation related to affective touch. This insightful dissociation seems crucial for a deeper understanding of the distinctive challenges characterizing people with ASD and may have implications for diagnosis and therapeutic approaches. Lay Summary: In the present study, we investigated the effects of affective touch on adult individuals with ASD from both an implicit and explicit perspective, integrating behavioral and physiological measures. Our results reveal that ASD individuals show a noteworthy discrepancy between explicit and implicit experience, characterized by the co‐occurrence of amplified hedonic and unpleasant ratings together with a lack of autonomic activation related to affective touch. This dissociation seems crucial for a deeper understanding of the distinctive challenges characterizing this syndrome and may have implications for diagnosis and therapeutic approaches. [ABSTRACT FROM AUTHOR]

Published
2024
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33. The Athena X-ray Integral Field Unit (X-IFU)

Author

Pajot, F., Barret, D., Lam-Trong, T., den Herder, J.-W., Piro, L., Cappi, M., Huovelin, J., Kelley, R., Mas-Hesse, J. M., Mitsuda, K., Paltani, S., Rauw, G., Rozanska, A., Wilms, J., Barbera, M., Douchin, F., Geoffray, H., den Hartog, R., Kilbourne, C., Le Du, M., Macculi, C., Mesnager, J.-M., and Peille, P.

Published
2018
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38. Immaginare l’altrove nell’epoca dell’Antropocene

Author

CAPPI, VALENTINA

Subjects
Imaginaries, Borders, Climate change, Media, Europe, Africa, thema EDItEUR::R Earth Sciences, Geography, Environment, Planning::RN The environment::RNP Pollution and threats to the environment::RNPG Climate change, thema EDItEUR::J Society and Social Sciences::JH Sociology and anthropology::JHB Sociology
Abstract

This book explores the processes through which particular places take shape in the imaginaries, perceptions and narratives of people who do not inhabit them, or who have inhabited them only recently. The ways in which we imagine the elsewhere are the product of stories collectively constructed and reproduced by a multiplicity of actors and through a variety of communicative tools and practices. These narratives shape our perceptions of others, the way we relate to them, and the politics that regulate cohabitation on Earth. In this book, the elsewhere becomes a device for exploring some of the ways in which human beings interact with each other, establish distinctions and alliances, trace borders, and enact change in the epoch of the Anthropocene. Through four phenomenologies of the elsewhere (Europe, Africa, the transnational space, climate change), the author reflects on the opportunity to decentralize one’s own gaze, in time and space, in order to imagine other ways of worldmaking.

Published
2023

42. O PROCESSO DE POSITIVAÇÃO DAS OBRIGAÇÕES TRIBUTÁRIAS ACESSÓRIAS - 10.12818/P.0304-2340.2017v71p143

Author

Fernando de Brito Alves and Tiago Cappi Janini

Subjects
Law in general. Comparative and uniform law. Jurisprudence, K1-7720
Abstract

A complexidade do direito, representada no fluxo da causalidade jurídica, implica normas derivadas de outras normas, até se chegar às individuais e concretas. Para analisar esse fenômeno de positivação de normas, optou-se pelas obrigações tributárias acessórias, com o propósito de desenvolver toda sua cadeia normativa. Valendo-se do método dedutivo e do método analítico, com apoio na pesquisa bibliográfica, legislativa e jurisprudencial, este texto tem como propósito analisar o processo de positivação referente às normas que tratam das obrigações acessórias tributárias. Com isso, procurar-se-á identificar qual a espécie de norma é competente para institui-las. Desse modo, estudar-se-á em que consiste o processo de positivação de normas, as obrigações acessórias dentro do sistema jurídico tributário e as teorias que tratam das possibilidades normativas para a criação das obrigações acessórias. Por fim, a partir da conclusão que é possível um ato infralegal instituir nova obrigação acessória no sistema jurídico, propõe-se um processo de positivação das suas normas, partindo-se dos dispositivos constitucionais até atingir esses deveres de fazer concretos elaborados pelo contribuinte, demonstrando-o com a Escrituração Contábil Digital (ECD) integrante do Sistema Público de Escrituração Digital (SPED).

Published
2018

43. Copy Number Variation in Obsessive-Compulsive Disorder and Tourette Syndrome: A Cross-Disorder Study

Author

McGrath, Lauren M., Yu, Dongmei, Marshall, Christian, Davis, Lea K., Thiruvahindrapuram, Bhooma, Li, Bingbin, Cappi, Carolina, Gerber, Gloria, Wolf, Aaron, Schroeder, Frederick A., Osiecki, Lisa, O'Dushlaine, Colm, Kirby, Andrew, Illmann, Cornelia, Haddad, Stephen, Gallagher, Patience, Fagerness, Jesen A., Barr, Cathy L., Bellodi, Laura, Benarroch, Fortu, Bienvenu, O. Joseph, Black, Donald W., Bloch, Michael H., Bruun, Ruth D., Budman, Cathy L., Camarena, Beatriz, Cath, Danielle C., Cavallini, Maria C., Chouinard, Sylvain, Coric, Vladimir, Cullen, Bernadette, Delorme, Richard, Denys, Damiaan, Derks, Eske M., Dion, Yves, Rosário, Maria C., Eapen, Valsama, Evans, Patrick, Falkai, Peter, Fernandez, Thomas V., Garrido, Helena, Geller, Daniel, Grabe, Hans J., Grados, Marco A., Greenberg, Benjamin D., Gross-Tsur, Varda, Grünblatt, Edna, Heiman, Gary A., Hemmings, Sian M.J., Herrera, Luis D., Hounie, Ana G., Jankovic, Joseph, Kennedy, James L., King, Robert A., Kurlan, Roger, Lanzagorta, Nuria, Leboyer, Marion, Leckman, James F., Lennertz, Leonhard, Lochner, Christine, Lowe, Thomas L., Lyon, Gholson J., Macciardi, Fabio, Maier, Wolfgang, McCracken, James T., McMahon, William, Murphy, Dennis L., Naarden, Allan L., Neale, Benjamin M., Nurmi, Erika, Pakstis, Andrew J., Pato, Michele T., Pato, Carlos N., Piacentini, John, Pittenger, Christopher, Pollak, Yehuda, Reus, Victor I., Richter, Margaret A., Riddle, Mark, Robertson, Mary M., Rosenberg, David, Rouleau, Guy A., Ruhrmann, Stephan, Sampaio, Aline S., Samuels, Jack, Sandor, Paul, Sheppard, Brooke, Singer, Harvey S., Smit, Jan H., Stein, Dan J., Tischfield, Jay A., Vallada, Homero, Veenstra-VanderWeele, Jeremy, Walitza, Susanne, Wang, Ying, Wendland, Jens R., Shugart, Yin Yao, Miguel, Euripedes C., Nicolini, Humberto, Oostra, Ben A., Moessner, Rainald, Wagner, Michael, Ruiz-Linares, Andres, Heutink, Peter, Nestadt, Gerald, Freimer, Nelson, Petryshen, Tracey, Posthuma, Danielle, Jenike, Michael A., Cox, Nancy J., Hanna, Gregory L., Brentani, Helena, Scherer, Stephen W., Arnold, Paul D., Stewart, S. Evelyn, Mathews, Carol A., Knowles, James A., Cook, Edwin H., Pauls, David L., Wang, Kai, and Scharf, Jeremiah M.

Published
2014
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44. The (in)visible Brazilians: A perspective review on the need for brain health and dementia research with Brazilian immigrants in the United States.

Author

Simon, Sharon Sanz, Brucki, Sonia Maria Dozzi, Fonseca, Luciana Mascarenhas, Becker, Jacqueline, Cappi, Carolina, Marques, Andrea Horvath, Heyn, Patricia C., Gonçalves, Priscila Dib, Martins, Silvia S., Busatto, Geraldo, Suemoto, Claudia Kimie, Nitrini, Ricardo, Caramelli, Paulo, Yassuda, Monica Sanches, Miotto, Eliane Correa, Grinberg, Lea Tenenholz, Arce Renteria, Miguel, Alegria, Margarita, Stern, Yaakov, and Rivera‐Mindt, Monica

Subjects
ALZHEIMER'S disease, HEALTH services accessibility, PUBLIC health research, SCIENTIFIC literature, BRAZILIANS, EMIGRATION & immigration
Abstract

Introduction: The Brazilian population in the United States (U.S.), a Latinx subgroup, is rapidly growing and aging but remains underrepresented in U.S. health research. In addition to group‐specific genetic and environmental risks, Brazilian immigrants and their offspring in the U.S. likely have cumulative risks for health inequities. It is estimated that 71% of Brazilian immigrants in the U.S. are undocumented, which may limit healthcare access/utilization. Furthermore, mental health is reported as a health priority by Brazilian immigrants in the U.S., and there is a lack of research on Alzheimer's disease and related dementia (AD/ADRD) in this population. Methods: We reviewed the scientific literature using traditional (e.g., PubMed) sources and databases generated by U.S. and Brazilian governments, as well as international organizations, and press articles. Results: This perspective review lists recommendations for researchers, health providers, and policymakers to promote greater inclusion of U.S. Brazilian populations in health research and care. The review identifies research areas in need of attention to address health inequities and promote mental/brain health in Brazilian immigrants and their offspring living in the U.S. These research areas are: 1) epidemiological studies to map the prevalence and incidence of mental/brain health conditions; 2) research on aging and AD/ADRD risk factors among Brazilian populations in the U.S.; and 3) the need for greater representation of U.S‐residing Brazilian population in other relevant research areas involving genetics, neuropathology, and clinical trials. Conclusions: The recommendation and research efforts proposed should help to pave the way for the development of community‐engagement research and to promote mental/brain health education, improvement of mental/brain health and AD/ADRD services, and the development of culturally‐informed intervention to the U.S.‐residing Brazilian communities. HIGHLIGHTS: The Brazilian population in the United States is growing but is underrepresented in U.S. health research.Approximately 71% of Brazilian immigrants in the United States are undocumented, with an increased risk for health inequities.Mental health is reported as a central health priority by Brazilian immigrants in the United States.There is a lack of research on Alzheimer's disease and other dementias (ADRD) in Brazilian immigrants in the United States.Epidemiological research is needed to map the prevalence/incidence of mental health conditions and ADRD risk factors among Brazilian immigrants in the United States. [ABSTRACT FROM AUTHOR]

Published
2023
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46. A Clinical and Angiographic Study of the XIENCE V Everolimus-Eluting Coronary Stent System in the Treatment of Patients With Multivessel Coronary Artery Disease: The EXECUTIVE Trial (EXecutive RCT: Evaluating XIENCE V in a Multi Vessel Disease)

Author

Ribichini, Flavio, Romano, Michele, Rosiello, Renato, La Vecchia, Luigi, Cabianca, Ester, Caramanno, Giuseppe, Milazzo, Diego, Loschiavo, Paolo, Rigattieri, Stefano, Musarò, Salvatore, Pironi, Bruno, Fiscella, Antonio, Amico, Francesco, Indolfi, Ciro, Spaccarotella, Carmen, Bartorelli, Antonio, Trabattoni, Daniela, Della Rovere, Francesco, Rolandi, Andrea, Beqaraj, Federico, Belli, Riccardo, Sangiorgio, Pietro, Villani, Rosvaldo, Berni, Andrea, Sheiban, Imad, Lopera Quijada, Maria Josè, Cappi, Barbara, Ribaldi, Licia, and Vassanelli, Corrado

Published
2013
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48. Tracking the spectral properties of ESO 511-G030 across different epochs.

Author

Middei, R., Petrucci, P.-O., Bianchi, S., Ursini, F., Matzeu, G. A., Vagnetti, F., Tortosa, A., Marinucci, A., Matt, G., Piconcelli, E., De Rosa, A., De Marco, B., Reeves, J., Perri, M., Guainazzi, M., Cappi, M., and Done, C.

Subjects
SPECTRAL energy distribution, ACTIVE galactic nuclei, SUPERMASSIVE black holes, SOLAR flares, ACCRETION (Astrophysics), MOLECULAR spectra
Abstract

The Type 1 active galactic nucleus (AGN) ESO 511-G030, a formerly bright and soft excess dominated source, was observed in 2019 in the context of a multi-wavelength monitoring campaign. In the new exposures, the source was found to be in a flux state approximately ten times lower than archival exposures and without any trace of the soft excess. Interestingly, the X-ray weakening observed in the 2019 data corresponds to a comparable fading of the UV flux, suggesting a strong link between these two components. The UV-X-ray spectral energy distribution (SED) of ESO 511-G030 shows remarkable variability. We tested both phenomenological and physically motivated models on the data, finding that the overall emission spectrum of ESO 511-G030 in this extremely low flux state is due to the superposition of a power-law-like continuum (1:7) and two reflection components emerging from hot and cold matter. Both the primary X-ray continuum and relativistic reflection are produced in the inner regions close to the supermassive black hole. The prominent variability of ESO 511-G030 and the lack of a soft excess can be explained by the dramatic change in the observed accretion rate, which dropped from an L=LEdd of 2% in 2007 to one of 0.2% in 2019. The X-ray photon index also became harder during the low flux observations from 2019, perhaps as a result of a photon starved X-ray corona. [ABSTRACT FROM AUTHOR]

Published
2023
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50. The VVDS Data‐Reduction Pipeline: Introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface

Author

Scodeggio, M., Franzetti, P., Garilli, B., Zanichelli, A., Paltani, S., Maccagni, D., Bottini, D., Le Brun, V., Contini, T., Scaramella, R., Adami, C., Bardelli, S., Zucca, E., Tresse, L., Ilbert, O., Foucaud, S., Iovino, A., Merighi, R., Zamorani, G., Gavignaud, I., Rizzo, D., McCracken, H. J., Le Fèvre, O., Picat, J. P., Vettolani, G., Arnaboldi, M., Arnouts, S., Bolzonella, M., Cappi, A., Charlot, S., Ciliegi, P., Guzzo, L., Marano, B., Marinoni, C., Mathez, G., Mazure, A., Meneux, B., Pellò, R., Pollo, A., Pozzetti, L., and Radovich, M.

Published
2005
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