Accès ouvert déclaré
2025
article
Euclid
F. J. Castander, P. Fosalba, J. Stadel, D. Potter, J. Carretero, i, L. Pozzetti, M. Bolzonella, G. A. Mamon, L Blot, Kai Hoffmann, P. Monaco, Elizabeth Johana Gonzalez, G. De Lucia, Claudia Scarlata, Michel-Andrès Breton, Laila Linke, C. Viglione, Shangrong Li, Zhongxu Zhai, Zahra Baghkhani, Kevin Pardede, C. Neissner, R Teyssier, M. Crocce, I. Tutusaus, L. Miller, G. Congedo, A. Biviano, M. Hirschmann, A Pezzotta, H. Aussel, Henk Hoekstra, T. Kitching, Will J. Percival, L. Guzzo, Y. Mellier, Pascal A. Oesch, R. A. A. Bowler, S Bruton, V. Allevato, Violeta González-Pérez, Marc Manera, S. Àvila, András Kovács, N. Aghanim, B. Altieri, A Amara, L. Amendola, S. Andreon, N. Auricchio, C. Baccigalupi, M. Baldi, A. Balestra, S. Bardelli, R. Bender, F. Bernardeau, C. Bodendorf, D. Bonino, E. Branchini, M. Brescia, J. Brinchmann, S. Camera, V. Capobianco, C. Carbone, S Casas, M. Castellano, G. Castignani, S. Cavuoti, A. Cimatti, C. Colodro-Conde, Christopher J. Conselice, L. Conversi, Y. Copin, L. Corcione, F. Courbin, H. M. Courtois, A. Da Silva, H. Degaudenzi, A. M. Di Giorgio, J. Dinis, M. Douspis, F. Dubath, C. A. J. Duncan, X. Dupac, S Dusini, A. Ealet, M. Farina, S. Farrens, S. Ferriol, S. Fotopoulou, N. Fourmanoit, M. Frailis, E. Franceschi, P. Franzetti, S. Galeotta, W. Gillard, B. Gillis, C. Giocoli, P. Gómez-Álvarez, B. R. Granett, A. Grazian, F. Grupp, S. V. H. Haugan, M. S. Holliman, W. Holmes, I. Hook, F. Hormuth, A. Hornstrup, P. Hudelot, S. Ilić, K. Jahnkę, M. Jhabvala, B Joachimi, E. Keihänen, S. Kermiche, A. Kiessling, M. Kilbinger, R. Kohley, B. Kubik, M Kümmel, M Kunz, H. Kurki‐Suonio, O. Lahav, R. Laureijs, D. Le Mignant, P. Liebing, S Ligori, P. B. Lilje, V. Lindholm, I. Lloro, D. Maino, E Maiorano, O. Mansutti, S. Marcin, O. Marggraf, K. Markovič, M. Martinelli, N. Martinet, F. Marulli, R Massey, Daniel Masters, S. Maurogordato, H. J. McCracken, E. Medinaceli, S Mei, M. Melchior, M. Meneghetti, E. Merlin, G. Meylan, J. J. Mohr, M. Moresco, L. Moscardini, E. Munari, R. Nakajima, R. C. Nichol, S.-M Niemi, C. Padilla, K. Paech, S. Paltani, F. Pasian, J. A. Peacock, K. Pedersen, V. Pettorino, S. Pires, G. Polenta, M. Poncet, Popa L, F. Raison, R. Rebolo, A. Renzi, J. Rhodes, G. Riccio, E. Romelli, M. Roncarelli, C. Rosset, E. Rossetti, B. Rusholme, R. Saglia, Z. Sakr, Ariel G. Sánchez, D. Sapone, Schewtschenko J, M. Schirmer, Peter Schneider, T. Schrabback, M. Scodeggio, A. Secroun, E. Sefusatti, G. Seidel, S. Serrano, C. Sirignano, G. Sirri, L. Stanco, Jean‐Luc Starck, J. Steinwagner, A. N. Taylor, Harry I. Teplitz, I. Tereno, R. Toledo-Moreo, F. Torradeflot, A. Tsyganov, L. Valenziano, T. Vassallo, A. Veropalumbo, Yun Wang, J. Weller, A. Zacchei, G. Zamorani, F. M. Zerbi, J. Zoubian, E Zucca, A. Boucaud, E. Bozzo, C. Burigana, M. Calabrese, P Casenove, D. Di Ferdinando, J. A. Escartin Vigo, G. Fabbian, F. Finelli⋆, J. Gracia-Carpio, S. Matthew, N. Mauri, M. Pöntinen, C. Porciani, V. Scottez, M. Tenti, M Viel, M. Wiesmann, Y. Akrami, S Anselmi, M. Archidiacono, F. Atrio‐Barandela, É. Aubourg, A. Balaguera-Antolínez, M Ballardini, Daniele Bertacca, M. Béthermin, Alain Blanchard, H. Böhringer, S Borgani, T. Bouvard, R Cabanac, Antonello Calabrò, B. Camacho Quevedo, G Cañas-Herrera, A. Cappi, F Caro, Carvalho C, T. Castro, K. C. Chambers, S. Contarini, T. Contini, Asantha Cooray, M. Costanzi, O. Cucciati, S. Davini, B. De Caro, S. de la Torre, G. Desprez, A. Díaz‐Sánchez, J.J Diaz, S. Di Domizio, H. Dole, S. Escoffier, M. Ezziati, A.G Ferrari, Pedro G. Ferreira, I. Ferrero, A. Finoguenov, A. Fontana, F. Fornari, L. Gabarra, K. Ganga, J. García-Bellido, T Gasparetto, E. Gaztañaga, F. Giacomini, F. Gianotti, Anthony H. Gonzalez, G. Gozaliasl, A Hall, W G Hartley, H. Hildebrandt, J. Hjorth, A. D. Holland, O. Ilbert, Shahab Joudaki, E. Jullo, J. J. E. Kajava, V. Kansal, D. Karagiannis, C. C. Kirkpatrick, J Le Graet, L Legrand, Julien Lesgourgues, T.I Liaudat, A. Loureiro, J. F. Macías–Pérez, M. Magliocchetti, C. Mancini, F. Mannucci, R. Maoli, C. J. A. P. Martins, L. Maurin, R. B. Metcalf, M. Migliaccio, M Miluzio, A. Mora, Claudio Moretti, G. Morgante, S. Nadathur, L. Nicastro, N. A. Walton, Masamune Oguri, L. Patrizii, V. Popa, A. Pourtsidou, P. Reimberg, I Risso, P.-F Rocci, R. P. Rollins, M Sahlén, J. Schaye, Aurel Schneider, M. Schultheis, M. Sereno, F. Shankar, A. Shulevski, Alessandra Silvestri, Pardis Simon, A. Spurio Mancini, S. A. Stanford, G. Testera, C. Tao, N Tessore, G. Testera, M. Tewes, Sune Toft, S. Tosi, A Troja, M. Tucci, C Valieri, J. Väliviita, D. Vergani, Filippo Vernizzi, G Verza, P Vielzeuf, John R. Weaver, L. Zalesky, Paola Dimauro, Pierre–Alain Duc, Y. Fang, A. M. N. Ferguson, C. M. Gutiérrez, I. Kovačić, Sandor Kruk, A.M.C Le Brun, A Montoro, Claire E. Murray, L. Pagano, D. Paoletti, E Sarpa, A. Viitanen, J Martín-Fleitas, D Scott, L. Y. Aaron Yung
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Le résumé fourni par la source
We present the Flagship galaxy mock, a simulated catalogue of billions of galaxies designed to support the scientific exploitation of the Euclid mission. Euclid is a medium-class mission of the European Space Agency optimised to determine the properties of dark matter and dark energy on the largest scales of the Universe. It probes structure formation over more than 10 billion years primarily from the combination of weak gravitational lensing and galaxy clustering data. The breadth of Euclid’s data will also foster a wide variety of scientific analyses. The Flagship simulation was developed to provide a realistic approximation to the galaxies that will be observed by Euclid and used in its scientific exploitation. We ran a state-of-the-art N-body simulation with four trillion particles, producing a lightcone on the fly. From the dark matter particles, we produced a catalogue of 16 billion haloes in one octant of the sky in the lightcone up to redshift z = 3. We then populated these haloes with mock galaxies using a halo occupation distribution and abundance-matching approach, calibrating the free parameters of the galaxy mock against observed correlations and other basic galaxy properties. Modelled galaxy properties include luminosity and flux in several bands, redshifts, positions and velocities, spectral energy distributions, shapes and sizes, stellar masses, star formation rates, metallicities, emission line fluxes, and lensing properties. We selected a final sample of 3.4 billion galaxies with a magnitude cut of HE < 26, where we are complete. We have performed a comprehensive set of validation tests to check the similarity to observational data and theoretical models. In particular, our catalogue is able to closely reproduce the main characteristics of the weak lensing and galaxy clustering samples to be used in the mission main cosmological analysis. Moreover, given its depth and completeness, this new galaxy mock also provides the community with a powerful tool for developing a wide range of scientific analyses beyond the Euclid mission.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Le contrôle bibliographique ouvert
DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.
- Titre Crossref
- <i>Euclid</i>
- Date Crossref
- 30/04/2025
- Éditeur
- EDP Sciences
- Type
- journal-article
Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.
Les sujets associés
Stellar, planetary, and galactic studiesAstronomy and Astrophysical ResearchAstronomical Observations and Instrumentation