Euclid: ESA's mission to map the geometry of the dark universe
Euclid: ESA's mission to map the geometry of the dark universe
复制标题
欧几里得:欧空局的使命是绘制黑暗宇宙的几何形状
DOI:
10.1117/12.926496
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发表时间:
2012
影响因子:
1.8
通讯作者:
L. Valenziano
中科院分区:
文献类型:
--
作者:
R. Laureijs;P. Gondoin;L. Duvet;G. S. Criado;J. Hoar;J. Amiaux;J. Auguères;R. Cole;M. Cropper;A. Ealet;P. Ferruit;I. E. Sanz;K. Jahnke;R. Kohley;T. Maciaszek;Y. Mellier;T. Oosterbroek;F. Pasian;M. Sauvage;R. Scaramella;M. Sirianni;L. Valenziano
Euclid is a space-borne survey mission developed and operated by ESA. It is designed to understand the origin of the Universe's accelerating expansion. Euclid will use cosmological probes to investigate the nature of dark energy, dark matter and gravity by tracking their observational signatures on the geometry of the Universe and on the history of structure formation. The mission is optimised for the measurement of two independent cosmological probes: weak gravitational lensing and galaxy clustering. The payload consists of a 1.2 m Korsch telescope designed to provide a large field of view. The light is directed to two instruments provided by the Euclid Consortium: a visual imager (VIS) and a near-infrared spectrometer-photometer (NISP). Both instruments cover a large common field of view of 0.54 deg2, to be able to survey at least 15,000 deg2 for a nominal mission of 6 years. An overview of the mission will be presented: the scientific objectives, payload, satellite, and science operations. We report on the status of the Euclid mission with a foreseen launch in 2019.