The Current Status of the Hard X-ray Modulation Telescope

被引:1
作者
Lu, Fangjun [1 ]
机构
[1] Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China
来源
SPACE TELESCOPES AND INSTRUMENTATION 2012: ULTRAVIOLET TO GAMMA RAY | 2012年 / 8443卷
关键词
X-ray; Scan Imaging; Timing;
D O I
10.1117/12.925620
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The Hard X-ray Modulation Telescope (HXMT) is China's first astronomical satellite. On board HXMT there are three kinds of slat-collimated telescopes, the High Energy X-ray Telescope (HE, 20-250 keV, 5000 cm(2)), the Medium Energy X-ray Telescope (ME, 5-30 keV, 952 cm(2)), and the Low Energy X-ray Telescope (LE, 1-15 keV, 394cm(2)). The typical Field of View (FOV) of HXMT is 1 degrees x6 degrees (FWHM), and it has other FOVs so as to measure the cosmic and the local particle induced X-ray backgrounds. The 3-sigma continuum sensitivity of HXMT is about 0.5 mCrab (10(5)s). HXMT will perform a broad band (1-250 keV) X-ray sky survey and do pointed observations of X-ray sources to study their broadband spectra and the multi-wavelength temporal variabilities. The planned launch date of HXMT is around 2014/2015. It will run in a low earth orbit with an inclination angle of 43 degrees, and its designed lifetime is 4 years. Now HXMT is in the pre-flight model construction phase
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页数:5
相关论文
共 3 条
[1]  
Craig W. W., 2005, Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, V5900, P266
[2]  
Fangjun L., 2009, AAPPS B, V19, P36
[3]  
Li Gang, 2008, Chinese Journal of Space Science, V28, P531