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26 April 2024
 
  » arxiv » 0809.1057

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The Wide-Field X and Gamma-Ray Telescope ECLAIRs aboard the Gamma-Ray Burst Multi-Wavelength Space Mission SVOM
P. Mandrou ; S. Schanne ; B. Cordier ; R. Pons ; D. Barret ; C. Amoros ; K. Lacombe ; M. Fesquet ; O. Limousin ; P. Sizun ; F. Lebrun ; F. Gonzalez ; M. Jouret ;
Date 5 Sep 2008
AbstractThe X and Gamma-ray telescope ECLAIRs is foreseen to be launched on a low Earth orbit (h=630 km, i=30 degrees) aboard the SVOM satellite (Space-based multi-band astronomical Variable Objects Monitor), a French-Chinese mission with Italian contribution. Observations are expected to start in 2013. It has been designed to detect and localize Gamma-Ray Bursts (GRBs) or persistent sources of the sky, thanks to its wide field of view (about 2 sr) and its remarkable sensitivity in the 4-250 keV energy range, with enhanced imaging sensitivity in the 4-70 keV energy band. These characteristics are well suited to detect highly redshifted GRBs, and consequently to provide fast and accurate triggers to other onboard or ground-based instruments able to follow-up the detected events in a very short time from the optical wavelength bands up to the few MeV Gamma-Ray domain.
Source arXiv, 0809.1057
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