Euclid preparation - VII. Forecast validation for Euclid cosmological probes

A. Blanchard; S. Camera; C. Carbone; V. F. Cardone; S. Casas; S. Clesse; S. Ilić; M. Kilbinger; T. Kitching; M. Kunz; F. Lacasa; E. Linder; E. Majerotto; K. Markovič; M. Martinelli; V. Pettorino; A. Pourtsidou; Z. Sakr; A. G. Sánchez; D. Sapone; I. Tutusaus; S. Yahia-Cherif; V. Yankelevich; S. Andreon; H. Aussel; A. Balaguera-Antolínez; M. Baldi; S. Bardelli; R. Bender; A. Biviano; D. Bonino; A. Boucaud; E. Bozzo; E. Branchini; S. Brau-Nogue; M. Brescia; J. Brinchmann; C. Burigana; R. Cabanac; V. Capobianco; A. Cappi; J. Carretero; C. S. Carvalho; R. Casas; F. J. Castander; M. Castellano; S. Cavuoti; A. Cimatti; R. Cledassou; C. Colodro-Conde; G. Congedo; C. J. Conselice; L. Conversi; Y. Copin; L. Corcione; J. Coupon; H. M. Courtois; M. Cropper; A. Da Silva; S. de la Torre; D. Di Ferdinando; F. Dubath; F. Ducret; C. A. J. Duncan; X. Dupac; S. Dusini; G. Fabbian; M. Fabricius; S. Farrens; P. Fosalba; S. Fotopoulou; N. Fourmanoit; M. Frailis; E. Franceschi; P. Franzetti; M. Fumana; S. Galeotta; W. Gillard; B. Gillis; C. Giocoli; P. Gómez-Alvarez; J. Graciá-Carpio; F. Grupp; L. Guzzo; H. Hoekstra; F. Hormuth; H. Israel; K. Jahnke; E. Keihanen; S. Kermiche; C. C. Kirkpatrick; R. Kohley; B. Kubik; H. Kurki-Suonio; S. Ligori; P. B. Lilje; I. Lloro; D. Maino; E. Maiorano; O. Marggraf; N. Martinet; F. Marulli; R. Massey; E. Medinaceli; S. Mei; Y. Mellier; B. Metcalf; J. J. Metge; G. Meylan; M. Moresco; L. Moscardini; E. Munari; R. C. Nichol; S. Niemi; A. A. Nucita; C. Padilla; S. Paltani; F. Pasian; W. J. Percival; S. Pires; G. Polenta; M. Poncet; L. Pozzetti; G. D. Racca; F. Raison; A. Renzi; J. Rhodes; E. Romelli; M. Roncarelli; E. Rossetti; R. Saglia; P. Schneider; V. Scottez; A. Secroun; G. Sirri; L. Stanco; J.-L. Starck; F. Sureau; P. Tallada-Crespí; D. Tavagnacco; A. N. Taylor; M. Tenti; I. Tereno; R. Toledo-Moreo; F. Torradeflot; L. Valenziano; T. Vassallo; G. A. Verdoes Kleijn; M. Viel; Y. Wang; A. Zacchei; J. Zoubian; E. Zucca

doi:10.1051/0004-6361/202038071

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Volume 642 (October 2020)

A&A, 642 (2020) A191

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Fig. 7.

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Marginalised 1σ errors on cosmological parameters (from the Fisher matrix for an indicative code), relative to their corresponding fiducial value for a flat (upper panels) and non-flat (lower panels) spatial geometry, in ΛCDM. Left (right) panels: pessimistic (optimistic) settings, as described in the text. Each histogram refers to different observational probes. For both a spatially flat and a spatially non-flat cosmology, we show results for GC_s, WL, GC_s+WL, GC_s+WL+GC_ph, and GC_s+WL+GC_ph+XC.

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