首页> 外文会议>2008 NanJing Gamma-Ray Burst Conference(2008年伽马暴国际研讨会)论文集 >The Wide-Field X and Gamma-Ray Telescope ECLAIRs aboard the Gamma-Ray Burst Multi-Wavelength Space Mission SVOM
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The Wide-Field X and Gamma-Ray Telescope ECLAIRs aboard the Gamma-Ray Burst Multi-Wavelength Space Mission SVOM

机译:伽玛射线暴多波长太空任务SVOM上的广角X和伽玛射线望远镜ECLAIR

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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.
机译:预计X和伽马射线望远镜ECLAIRs将在法中中文卫星SVOM卫星(天基多波段天文可变物体监视器)上的低地球轨道(h = 630 km,i = 30°)上发射。预计将在2013年开始进行观测(魏,J。,这些程序)。由于其广阔的视野,它的设计目的是探测和I灭伽玛射线暴(GRB)或持续存在的天空源( ≈2 sr)及其在4-250 keV能量范围内的出色灵敏度,在4-70 keV能量带内具有增强的成像灵敏度。这些特性非常适合检测高度红移的GRB,从而为其他机载板提供快速准确的触发或地面仪器,能够在很短的时间内跟踪从光学波长带到少数MeV伽马射线域的检测到的事件。

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