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A study of the pointed observation methods and sensitivity of HXMT

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【作者】 金晶陈勇张双南张澍李新乔李刚

【Author】 JIN Jing1,2;1) CHEN Yong3 ZHANG Shuang-Nan4,2,3 ZHANG Shu3 LI Xin-Qiao3 LI Gang3 1 Department of Engineering Physics, Tsinghua University, Beijing 100084, China 2 Center for Astrophysics, Tsinghua University, Beijing 100084, China 3 Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China 4 Department of Physics, Tsinghua University, Beijing 100084, China

【机构】 Department of Engineering Physics, Tsinghua UniversityCenter for Astrophysics, Tsinghua UniversityKey Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of SciencesDepartment of Physics, Tsinghua University

【摘要】 The Hard X-ray Modulation Telescope (HXMT) is an X-ray astronomy satellite consisting of three slat-collimated instruments, the High Energy X-ray Instrument (HE), the Medium Energy X-ray Instrument (ME), and the Low Energy X-ray Instrument (LE). HXMT will carry out an all sky survey and make pointed observations in the 1-250 keV energy band. In order to get the source and background fluxes simultaneously in the pointed observations, two methods, i.e., the combined field of view (FOV) method and the off-axis pointing method are proposed in this paper. Comprehensive analyses of the sensitivities of the three instruments by using these two methods are presented, respectively. It is found that the off-axis pointing method has a higher sensitivity for HE and ME but a lower sensitivity for LE. Since the axes of the three instruments are aligned along the same direction, the off-axis pointing method is recommended as the main method in the pointed observation for HXMT; the combined FOV method can be used when LE is the most relevant instrument in order to satisfy the scientific objective of the observation.

【Abstract】 The Hard X-ray Modulation Telescope (HXMT) is an X-ray astronomy satellite consisting of three slat-collimated instruments, the High Energy X-ray Instrument (HE), the Medium Energy X-ray Instrument (ME), and the Low Energy X-ray Instrument (LE). HXMT will carry out an all sky survey and make pointed observations in the 1–250 keV energy band. In order to get the source and background fluxes simultaneously in the pointed observations, two methods, i.e., the combined field of view (FOV) method and the off-axis pointing method are proposed in this paper. Comprehensive analyses of the sensitivities of the three instruments by using these two methods are presented, respectively. It is found that the off-axis pointing method has a higher sensitivity for HE and ME but a lower sensitivity for LE. Since the axes of the three instruments are aligned along the same direction, the off-axis pointing method is recommended as the main method in the pointed observation for HXMT; the combined FOV method can be used when LE is the most relevant instrument in order to satisfy the scientific objective of the observation.

【关键词】 HXMTpointed observationsensitivityoff-axis
【Key words】 HXMTpointed observationsensitivityoff-axis
【基金】 Supported by National Basic Research Program of China (973 Program 2009CB824800)
  • 【文献出处】 中国物理C ,Chinese Physics C , 编辑部邮箱 ,2010年01期
  • 【分类号】P111.4
  • 【被引频次】5
  • 【下载频次】49
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