A study of the pointed observation methods and sensitivity of HXMT

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...

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Published inChinese physics C Vol. 34; no. 1; pp. 66 - 71
Main Author 金晶 陈勇 张双南 张澍 李新乔 李刚
Format Journal Article
LanguageEnglish
Published IOP Publishing 2010
Department of Engineering Physics, Tsinghua University, Beijing 100084, China
Center for Astrophysics, Tsinghua University, Beijing 100084, China%Key Laboratory of Particle Astrophysics, Institute of High Energy Physics,Chinese Academy of Sciences, Beijing 100049, China%Department of Physics, Tsinghua University, Beijing 100084, China
Center for Astrophysics, Tsinghua University, Beijing 100084, China
Key Laboratory of Particle Astrophysics, Institute of High Energy
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ISSN1674-1137
0254-3052
2058-6132
DOI10.1088/1674-1137/34/1/012

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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.
AbstractList O4; 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.
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.
Author 金晶 陈勇 张双南 张澍 李新乔 李刚
AuthorAffiliation Department of Engineering Physics, Tsinghua University, Beijing 100084, China Center for Astrophysics, Tsinghua University, Beijing 100084, China Key Laboratory of Particle Astrophysics, Institute of High Energy Physics Chinese Academy of Sciences, Beijing 100049, China Department of Physics, Tsinghua University, Beijing 100084, China
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Department of Engineering Physics, Tsinghua University, Beijing 100084, China
Center for Astrophysics, Tsinghua University, Beijing 100084, China%Key Laboratory of Particle Astrophysics, Institute of High Energy Physics,Chinese Academy of Sciences, Beijing 100049, China%Department of Physics, Tsinghua University, Beijing 100084, China
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References Li Ti-Pei (1) 2006; 26
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Li Ti-Pei (2) 1994; 215
Rothschild R E (3) 1998; 496
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SubjectTerms X射线仪器
X射线天文卫星
低能量
敏感性分析
灵敏度
硬X射线调制望远镜
Title A study of the pointed observation methods and sensitivity of HXMT
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