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High Energy X-ray Telescope Data Analysis Method

ZHAO Haisheng LI Chengkui LI Xiaobo NIE Jianyin GE Mingyu PAN Yuanyue SONG Liming

ZHAO Haisheng, LI Chengkui, LI Xiaobo, NIE Jianyin, GE Mingyu, PAN Yuanyue, SONG Liming. High Energy X-ray Telescope Data Analysis Method[J]. 空间科学学报, 2016, 36(6): 938-944. doi: 10.11728/cjss2016.06.938
引用本文: ZHAO Haisheng, LI Chengkui, LI Xiaobo, NIE Jianyin, GE Mingyu, PAN Yuanyue, SONG Liming. High Energy X-ray Telescope Data Analysis Method[J]. 空间科学学报, 2016, 36(6): 938-944. doi: 10.11728/cjss2016.06.938
ZHAO Haisheng, LI Chengkui, LI Xiaobo, NIE Jianyin, GE Mingyu, PAN Yuanyue, SONG Liming. High Energy X-ray Telescope Data Analysis Method[J]. Chinese Journal of Space Science, 2016, 36(6): 938-944. doi: 10.11728/cjss2016.06.938
Citation: ZHAO Haisheng, LI Chengkui, LI Xiaobo, NIE Jianyin, GE Mingyu, PAN Yuanyue, SONG Liming. High Energy X-ray Telescope Data Analysis Method[J]. Chinese Journal of Space Science, 2016, 36(6): 938-944. doi: 10.11728/cjss2016.06.938

High Energy X-ray Telescope Data Analysis Method

doi: 10.11728/cjss2016.06.938
基金项目: 

Supported by the National Natural Science Foundation of China (11303027, 11503029), and the Strategic Priority Research Program on Space Science of the Chinese Academy of Sciences (XDA04010300)

详细信息
    通讯作者:

    ZHAO Haisheng,E-mail:E-mail:zhaohs@ihep.ac.cn

  • 中图分类号: V557

High Energy X-ray Telescope Data Analysis Method

Funds: 

Supported by the National Natural Science Foundation of China (11303027, 11503029), and the Strategic Priority Research Program on Space Science of the Chinese Academy of Sciences (XDA04010300)

  • 摘要: The science analysis of the data from the High Energy X-ray Telescope (HE) on the Hard X-ray Modulation Telescope (HXMT) satellite is organized in three stages: calibration, screening and extraction of high-level scientific products. At the first stage, the raw PHA value of each event is converted to PI value accounting for temporal changes in gain and energy offset. At the second stage, the calibrated events are screened by applying cleaning criteria. At the third stage, scientific products, i.e. spectra, light curves and redistribution matrix files, are extracted. This work will introduce the three stages as well as the screening criteria and the data combining method.

     

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    [11] ftools:A General Package of Software to Manipulate FITS Files[OL].[2016-05-11]. http://heasarc.gsfc.nasa.gov/ftools/
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    [14] NASA's HEASARC Software Packages[OL].[2014-03-11]. http://heasarc.gsfc.nasa.gov/docs/software.html
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出版历程
  • 收稿日期:  2015-08-24
  • 修回日期:  2016-03-17
  • 刊出日期:  2016-11-15

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