 |
Conference papers
Euclid mission: building of a reference survey
J. Amiaux
1
R. Scaramella
Y. Mellier
2
B. Altieri
C. Burigana
A. da Silva
P. Gomez
J. Hoar
R.- J. Laureijs
E. Maiorano
D. Magalhães Oliveira
F. Renk
G. Saavedra Criado
I. Tereno
J.-L. Auguères
1
J. Brinchmann
M. Cropper
L. Duvet
A. Ealet
3
P. Franzetti
B. Garilli
P. Gondoin
L. Guzzo
H. Hoekstra
R. Holmes
K. Jahnke
T. Kitching
M. Meneghetti
W. Percival
S. Warren
W. Percival
Author
S. Warren
Author
1
DAPNIA - Département d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée (France)
- CEA - Commissariat à l'énergie atomique et aux énergies alternatives : DSM/DAPNIA (Centre de Saclay Centre de Grenoble Centre de Cadarache etc - France)
2
IAP - Institut d'Astrophysique de Paris (98bis, bd Arago - 75014 Paris France - France)
- CNRS - Centre National de la Recherche Scientifique : UMR7095 (France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- UPMC - Université Pierre et Marie Curie - Paris 6 (4 place Jussieu - 75005 Paris - France)
3
CPPM - Centre de Physique des Particules de Marseille (163, avenue de Luminy - Case 902 - 13288 Marseille cedex 09 - France)
- AMU - Aix Marseille Université : UMR7346 / UMR6550 / UMR6450 / URA6450 (Aix-Marseille Université Jardins du Pharo 58 Boulevard Charles Livon 13284 Marseille cedex 7 - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- CNRS - Centre National de la Recherche Scientifique : UMR7346 / UMR6550 / UMR6450 / URA6450 (France)
Abstract : Euclid is an ESA Cosmic-Vision wide-field-space mission which is designed to understand the acceleration of the Universe's expansion. The mission relies on two primary cosmological probes: Weak gravitational Lensing (WL) and Galaxy Clustering (in particular Baryon Acoustic Oscillations, BAO). The construction of a Reference Survey derived from the high level science requirements, the definition of a main sequence of observation and the associated calibrations was indeed a major achievement of the Definition Phase. Implementation of this sequence demonstrated the feasibility of covering the requested area in less than 6 years while taking into account the overheads of space segment observing and maneuvering sequence.
Document type :
Conference papers
Domain :
Sciences of the Universe [physics] / Astrophysics [astro-ph] / Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics [physics] / Astrophysics [astro-ph] / Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Sciences of the Universe [physics] / Astrophysics [astro-ph] / Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics [physics] / Astrophysics [astro-ph] / Instrumentation and Methods for Astrophysic [astro-ph.IM]
Complete list of metadata
http://hal.in2p3.fr/in2p3-00716748
Contributor : Danielle Cristofol <>
Submitted on : Wednesday, July 11, 2012 - 11:07:07 AM
Last modification on : Tuesday, March 30, 2021 - 3:17:07 AM
Contributor : Danielle Cristofol <>
Submitted on : Wednesday, July 11, 2012 - 11:07:07 AM
Last modification on : Tuesday, March 30, 2021 - 3:17:07 AM
Identifiers
- HAL Id : in2p3-00716748, version 1
Collections
Citation
J. Amiaux, R. Scaramella, Y. Mellier, B. Altieri, C. Burigana, et al.. Euclid mission: building of a reference survey. Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave, Jul 2012, Amsterdam, Netherlands. pp.8442-32. ⟨in2p3-00716748⟩
Metrics
Record views