Euclid preparation - VII. Forecast validation for Euclid cosmological probes
- Blanchard A.
- Camera S.
- Carbone C.
- Cardone V. F.
- Casas S.
- Clesse S.
- Ilić S.
- Kilbinger M.
- Kitching T.
- Kunz M.
- Lacasa F.
- Linder E.
- Majerotto E.
- Markovič K.
- Martinelli M.
- Pettorino V.
- Pourtsidou A.
- Sakr Z.
- Sánchez A. G.
- Sapone D.
- Tutusaus I.
- Yahia-Cherif S.
- Yankelevich V.
- Andreon S.
- Aussel H.
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- Bonino D.
- Boucaud A.
- Bozzo E.
- Branchini E.
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- Burigana C.
- Cabanac R.
- Capobianco V.
- Cappi A.
- Carretero J.
- Carvalho C. S.
- Casas R.
- Castander F. J.
- Castellano M.
- Cavuoti S.
- Cimatti A.
- Cledassou R.
- Colodro-Conde C.
- Congedo G.
- Conselice C. J.
- Conversi L.
- Copin Y.
- Corcione L.
- Coupon J.
- Courtois H. M.
- Cropper M.
- Da Silva
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- D. Dubath
- F. Ducret
- F. Duncan
- C. A. J. Dupac
- X. Dusini
- S. Fabbian
- G. Fabricius
- M. Farrens
- S. Fosalba
- P. Fotopoulou
- S. Fourmanoit
- N. Frailis
- M. Franceschi
- E. Franzetti
- P. Fumana
- M. Galeotta
- S. Gillard
- W. Gillis
- B. Giocoli
- C. Gómez-Alvarez
- P. Graciá-Carpio
- J. Grupp
- F. Guzzo
- L. Hoekstra
- H. Hormuth
- F. Israel
- H. Jahnke
- K. Keihanen
- E. Kermiche
- S. Kirkpatrick
- C. C. Kohley
- R. Kubik
- B. Kurki-Suonio
- H. Ligori
- S. Lilje
- P. B. Lloro
- I. Maino
- D. Maiorano
- E. Marggraf
- O. Martinet
- N. Marulli
- F. Massey
- R. Medinaceli
- E. Mei
- S. Mellier
- Y. Metcalf
- B. Metge
- J. J. Meylan
- G. Moresco
- M. Moscardini
- L. Munari
- E. Nichol
- R. C. Niemi
- S. Nucita
- A. A. Padilla
- C. Paltani
- S. Pasian
- F. Percival
- W. J. Pires
- S. Polenta
- G. Poncet
- M. Pozzetti
- L. Racca
- G. D. Raison
- F. Renzi
- A. Rhodes
- J. Romelli
- E. Roncarelli
- M. Rossetti
- E. Saglia
- R. Schneider
- P. Scottez
- V. Secroun
- A. Sirri
- G. Stanco
- L. Starck
- J. -L.
- Sureau F.
- Tallada-Crespí P.
- Tavagnacco D.
- Taylor A. N.
- Tenti M.
- Tereno I.
- Toledo-Moreo R.
- Torradeflot F.
- Valenziano L.
- Vassallo T.
- Verdoes Kleijn
- G. A. Viel
- M. Wang
- Y. Zacchei
- A. Zoubian
- J. Zucca
DOIAbstract
Aims. The Euclid space telescope will measure the shapes and redshifts of galaxies to reconstruct the expansion history of the Universe and the growth of cosmic structures. The estimation of the expected performance of the experiment, in terms of predicted constraints on cosmological parameters, has so far relied on various individual methodologies and numerical implementations, which were developed for different observational probes and for the combination thereof. In this paper we present validated forecasts, which combine both theoretical and observational ingredients for different cosmological probes. This work is presented to provide the community with reliable numerical codes and methods for Euclid cosmological forecasts. Methods. ...
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