{"paper":{"title":"Euclid preparation. XXXIV. The effect of linear redshift-space distortions in photometric galaxy clustering and its cross-correlation with cosmic shear","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A.Amara, A.A.Nucita, A.Balaguera-Antol\\'inez, A.Biviano, A.Boucaud, A.Cappi, A.Cimatti, A.DaSilva, A.D\\'iaz-S\\'anchez, A.Grazian, A.G.S\\'anchez, A.Hornstrup, A.Kiessling, A.Loureiro, A.N.Taylor, A.Pezzotta, A.R.Cooray, A.Renzi, A.S.Borlaff, A.Schneider, A.Secroun, A.Spurio Mancini, A.Tramacere, A.Veropalumbo, B.Garilli, B.Gillis, B.Joachimi, B.Sartoris, C.Baccigalupi, C.Burigana, C.Carbone, C.C.Kirkpatrick, C.Colodro-Conde, C.Giocoli, C.J.A.P.Martins, C.Padilla, C.S.Carvalho, C.Sirignano, D.Benielli, D.Di Ferdinando, D.Potter, D.Sapone, E.A.Valentijn, E.Bozzo, E.Branchini, E.Franceschi, E.Gaztanaga, E.Keihanen, E.Maiorano, E.Medinaceli, E.Munari, E.Romelli, E.Rossetti, Euclid Collaboration: K.Tanidis, E.Zucca, F.Bernardeau, F.Courbin, F.Dubath, F.Finelli, F.Giacomini, F.Grupp, F.Marulli, F.Pasian, F.Raison, F.Torradeflot, G.Ca\\~nas-Herrera, G.Castignani, G.Congedo, G.DeLucia, G.Desprez, G.Gozaliasl, G.Mainetti, G.Meylan, G.Morgante, G.Polenta, G.Riccio, G.Seidel, G.Sirri, G.Zamorani, H.Degaudenzi, H.Dole, H.Hildebrandt, H.Kurki-Suonio, H.M.Courtois, I.Ferrero, I.Hook, I.Lloro, I.Tereno, I.Tutusaus, J.A.Escartin Vigo, J.A.Schewtschenko, J.Brinchmann, J.Carretero, J.Coupon, J.Dinis, J.E.Pollack, J.Garc\\'ia-Bellido, J.Graci\\'a-Carpio, J.J.E.Kajava, J.Macias-Perez, J.Rhodes, J.Steinwagner, J.Valiviita, J.Weller, J.Zoubian, K.C.Chambers, K.Jahnke, K.Markovic, K.Pedersen, L.A.Popa, L.Conversi, L.Corcione, L.Gabarra, L.Guzzo, L.Legrand, L.Linke, L.Maurin, L.Moscardini, L.Patrizii, L.Stanco, L.Valenziano, M.Baldi, M.Ballardini, M.Brescia, M.Castellano, M.Farina, M.Frailis, M.Fumana, M.Kunz, M.Magliocchetti, M.Martinelli, M.Meneghetti, M.Migliaccio, M.Moresco, M.Poncet, M.P\\\"ontinen, M.Roncarelli, M.Schirmer, M.Sereno, M.Tenti, M.Tewes, M.Viel, N.Aghanim, N.Auricchio, N.Martinet, N.Mauri, O.Mansutti, O.Marggraf, P.B.Lilje, P.Fosalba, P.G.Ferreira, P.Monaco, P.Schneider, P.Simon, P.Tallada-Cresp\\'i, R.B.Metcalf, R.Cabanac, R.Cledassou, R.Farinelli, R.Maoli, R.Massey, R.Saglia, R.Teyssier, R.Toledo-Moreo, S.Andreon, S.Bardelli, S.Borgani, S.Camera, S.Casas, S.Cavuoti, S.Davini, S.delaTorre, S.DiDomizio, S.Dusini, S.Escoffier, S.Farrens, S.Ferriol, S.Galeotta, S.Ili\\'c, S.Kermiche, S.Marcin, S.Matthew, S.Maurogordato, S.Mei, S.-M.Niemi, S.Nadathur, S.Paltani, S.Pires, S.Serrano, S.Toft, S.V.H.Haugan, T.Castro, T.Vassallo, V.Allevato, V.Capobianco, V.F.Cardone, V.Kansal, V.Lindholm, V.Pettorino, V.Popa, V.Scottez, W.Gillard, W.Holmes, W.J.Percival, X.Dupac, Y.Akrami, Y.Copin, Y.Wang, Z.Sakr","submitted_at":"2023-08-31T18:00:07Z","abstract_excerpt":"The cosmological surveys that are planned for the current decade will provide us with unparalleled observations of the distribution of galaxies on cosmic scales, by means of which we can probe the underlying large-scale structure (LSS) of the Universe. This will allow us to test the concordance cosmological model and its extensions. However, precision pushes us to high levels of accuracy in the theoretical modelling of the LSS observables, so that no biases are introduced into the estimation of the cosmological parameters. In particular, effects such as redshift-space distortions (RSD) can bec"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2309.00052","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2309.00052/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}