The Wide-Field X and Gamma-Ray Telescope ECLAIRs aboard the Gamma-Ray Burst Multi-Wavelength Space Mission SVOM
The X and Gamma-ray telescope ECLAIRs is foreseen to be launched on a low Earth orbit(h=630 km,i=30°)aboard the SVOM satellite (Space-based multi-band astronomical Variable Objects Monitor),a French-Chinese missionwith Italian contribution．Observations are expected to start in 2013(Wei,J．,these proceedings)．It has been designed todetect and Iocalize Gamma-Ray Bursts(GRBs)or persistent sources of the sky,thanks to its wide field of view(≈2 sr)and its remarkable sensitivity in the 4-250 keV energy range,with enhanced imaging sensitivity in the 4-70 keV energyband．These characteristics arc well suited to detect highly redshifted GRBs,and consequently to provide fast andaccurate triggers to other onboard or ground-based instruments able tO follow-up the detected events in a very short timefrom the optical wavelength bands up to the few MeV Gamma-Ray domain.
SVOM ECLAlRs Gamma-Ray bursts gamma-ray telescopes CdTe
P.Mandrou P.Sizun F.Lebrun F.Gonzalez M.Jouret S.Schanne B.Cordier R.Pons D.Barret C.Amoros K.Lacombe M.Fesquet O.Limousin
CESR/CNRS/UPS,9 Avenue Colonel Roche,BP 44346,31028 Toulouse,Cedex 4,France CEA Saclay,DSM/IRFU(former DAPNIA),91191 Gif sur Yvette Cedex,France CEA Saclay,DSM/IRFU(former DAPNIA),91191 Gif sur Yvette Cedex,France APC 10 Rue Alice Domont et Leo CNES,CST,18 Avenue Edouard Belin,31401 Toulouse Cedex 9,France CEA Saclay,DSM/IRFU(former APNIA),91191 Gif sur Yvette Cedex,France
国际会议
2008 NanJing Gamma-Ray Burst Conference(2008年伽马暴国际研讨会)
南京
英文
338-341
2008-06-23（万方平台首次上网日期，不代表论文的发表时间）