Euclid space mission: a cosmological challenge for the next 15 years. Issue Volume 10:Issue S306(2014) (1st July 2015)

• Record Type: Journal Article
• Authors: Scaramella, R.; Mellier, Y.; Amiaux, J.; Burigana, C.; Carvalho, C.S.; Cuillandre, J.C.; da Silva, A.; Dinis, J.; Derosa, A.; Maiorano, E.; Franzetti, P.; Garilli, B.; Maris, M.; Meneghetti, M.; Tereno, I.; Wachter, S.; Amendola, L.; Cropper, M.; Cardone, V.; Massey, R.; Niemi, S.; Hoekstra, H.; Kitching, T.; Miller, L.; Schrabback, T.; Semboloni, E.; Taylor, A.; Viola, M.; Maciaszek, T.; Ealet, A.; Guzzo, L.; Jahnke, K.; Percival, W.; Pasian, F.; Sauvage, M.;
• Editors: Heavens, A. F.; Starck, J.-L.; Krone-Martins, A.
• Is Part Of: Proceedings of the International Astronomical Union. Volume 10:Issue S306(2014)
• Page Start: 375
• Page End: 378
• Publication Date: 2015-07-01
• Subjects: cosmology: cosmological parameters, -- gravitational lensing, -- dark matter, -- large-scale structure of universe; Astronomy -- Congresses; Astronomy -- Periodicals; 520
• DOI: 10.1017/S1743921314011089
• Languages: English
• ISSNs: 1743-9213

Abstract

Abstract: Euclid is the next ESA mission devoted to cosmology. It aims at observing most of the extragalactic sky, studying both gravitational lensing and clustering over ~15, 000 square degrees. The mission is expected to be launched in year 2020 and to last six years. The sheer amount of data of different kinds, the variety of (un)known systematic effects and the complexity of measures require efforts both in sophisticated simulations and techniques of data analysis. We review the mission main characteristics, some aspects of the the survey and highlight some of the areas of interest to this meeting.