{"paper":{"title":"$Euclid$ preparation: XV. Forecasting cosmological constraints for the $Euclid$ and CMB joint analysis","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. Blanchard, A. Cappi, A. Cimatti, A. Costille, A. Da Silva, A. Ealet, A. Grazian, A. Gruppuso, A.G. S\\'anchez, A. Kiessling, A.N. Taylor, A. Pourtsidou, A. Renzi, A. Secroun, A. Tramacere, A. Zacchei, B. Garilli, B. Gillis, B. Kubik, B. Morin, C.A.J. Duncan, C. Baccigalupi, C. Bodendorf, C. Burigana, C. Carbone, C.C. Kirkpatrick, C. Colodro-Conde, C. Giocoli, C. Hern\\'andez-Monteagudo, C.J. Conselice, C. Neissner, C. Padilla, C. Rosset, C.S. Carvalho, C. Sirignano, D. Bonino, D. Di Ferdinando, D. Maino, D. Marinucci, D. Paoletti, D. Potter, D. Sapone, E.A. Valentijn, E. Bozzo, E. Branchini, E. Franceschi, E. Keihanen, E. Medinaceli, E. Merlin, E. Munari, E. Romelli, E. Rossetti, Euclid Collaboration: S. Ili\\'c, E. Zucca, F. Dubath, F. Finelli, F. Grupp, F. Hormuth, F.J. Castander, F. Lacasa, F. Marulli, F. Pasian, F. Raison, F. Sureau, F. Torradeflot, G.A. Verdoes Kleijn, G. Castignani, G. Congedo, G. Fabbian, G. Gozaliasl, G. Mainetti, G. Meylan, G. Morgante, G. Polenta, G. Riccio, G. Seidel, G. Sirri, G. Zamorani, H. Degaudenzi, H. Dole, H. Hoekstra, H. Kurki-Suonio, H.M. Courtois, I. Lloro, I. Tereno, I. Tutusaus, J. Brinchmann, J. Carretero, J. Coupon, J. Cuby, J. Graci\\'a-Carpio, J.L. Starck, J. Nightingale, J.R. Bermejo-Climent, J. Rhodes, J. Valiviita, J. Weller, J. Zoubian, K. Ganga, K. Jahnke, K. Markovic, K. Pedersen, L. Conversi, L. Corcione, L. Guzzo, L. Legrand, L. Moscardini, L. Pagano, L. Patrizii, L. Popa, L. Pozzetti, L. Stanco, L. Valenziano, L. Wenzl, L. Whittaker, M. Archidiacono, M. Baldi, M. Ballardini, M. Brescia, M. Castellano, M. Cropper, M. Douspis, M. Farina, M. Frailis, M. Fumana, M. Kilbinger, M. K\\\"ummel, M. Kunz, M. Langer, M. Lattanzi, M. Martinelli, M. Maturi, M. Meneghetti, M. Migliaccio, M. Moresco, M. Poncet, M. Roncarelli, M. Schirmer, M. Schultheis, M. Tenti, M. Viel, N. Aghanim, N. Auricchio, N. Martinet, N. Mauri, N. Welikala, O. Mansutti, O. Marggraf, P. B. Lilje, P. Flose-Reimberg, P. Fosalba, P. Franzetti, P.G. Ferreira, P. Hudelot, P. Natoli, P. Ntelis, P. Schneider, P. Tallada-Cresp\\'i, P. Vielzeuf, R. Bender, R.B. Metcalf, R. Cabanac, R. Cledassou, R. Kohley, R. Laureijs, R. Massey, R. Rebolo, R. Saglia, R. Scaramella, R. Teyssier, R. Toledo-Moreo, S. Andreon, S. Bardelli, S. Borgani, S. Camera, S. Casas, S. Cavuoti, S. de la Torre, S. Dusini, S. Farrens, S. Galeotta, S. Kermiche, S. Ligori, S. Maurogordato, S. Mei, S.M. Niemi, S. Paltani, S. Pires, S. Serrano, S.V.H. Haugan, T. Kitching, T. Vassallo, V. Capobianco, V.F. Cardone, V. Lindholm, V. Pettorino, V. Scottez, V. Yankelevich, W. Gillard, W. Holmes, W. Percival, X. Dupac, Y. Copin, Y. Wang, Z. Sakr","submitted_at":"2021-06-15T18:00:57Z","abstract_excerpt":"The combination and cross-correlation of the upcoming $Euclid$ data with cosmic microwave background (CMB) measurements is a source of great expectation since it will provide the largest lever arm of epochs, ranging from recombination to structure formation across the entire past light cone. In this work, we present forecasts for the joint analysis of $Euclid$ and CMB data on the cosmological parameters of the standard cosmological model and some of its extensions. This work expands and complements the recently published forecasts based on $Euclid$-specific probes, namely galaxy clustering, we"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2106.08346","kind":"arxiv","version":2},"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/2106.08346/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"}