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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]. 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]. 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.

     

  • [1] LI Tipei, WU Mei. The hard X-ray modulation telescope mission[J]. Physics, 2008, 37(9):648-651
    [2] LI Tipei. HXMT:a Chinese high-energy astrophysics mission[J]. Nucl. Phys.:B, 2007,166:131-139
    [3] WELLS D C, GREISEN E W, HARTEN R H. FITS:A Flexible Image Transport System[R]. AAS, 1981, 44:363-370
    [4] MCGLYNN T A. A Primer on the FITS Data Format[R/OL].[2014-10-28]. http://fits.gsfc.nasa.gov/fits_primer.html.
    [5] SMITH E, STARK M, GILES B. South Atlantic anomaly entry and exit as measured by the X-ray timing explorer[C]//NASA Conference Publication, Flight Mechanics/Estimation THeory Symposium, 1996:249-256
    [6] Institute of Space and Astronautical Science (ISAS/JAXA) and the X-ray Astrophysics Laboratory in NASA/Goddard Space Flight Center, The Suzaku Data Reduction Guide[R/OL].[2013-09-04]. http://heasarc.gsfc.nasa.gov/docs/suzaku/analysis/abc/
    [7] Laboratory for High Energy Astrophysics in NASA/Goddard Space Flight Center, ASCA ABS Guide[R/OL].[1997-05-07]. http://www.astropa.unipa.it/SERVICES/ASCA/doc/html/ABC/node6.html
    [8] ARNAUD K, DORMAN B, GORDON C. Xspec:An X-ray Spectral Fitting Package[R/OL].[15-07-29]. http://heasarc.gsfc.nasa.gov/docs/xanadu/xspec/index.html
    [9] Xronos:A Timing Analysis Software Package[OL].[2009-08-21].http://heasarc.gsfc.nasa.gov/docs/xanadu/xronos/xronos.html
    [10] David Huenemoerder, John Davis, John Houck, Mike Nowak. How to and Why (or why not) combine Data[R/OL].[2011-05-31]. http://cxc.harvard.edu/ciao/download/doc/combine.pdf
    [11] ftools:A General Package of Software to Manipulate FITS Files[OL].[2016-05-11]. http://heasarc.gsfc.nasa.gov/ftools/
    [12] LI Gang, WU Mei, ZHANG Shu, JIN Yingkang. Space environment background calculation for HXMT[J]. Chin. J. Space Sci., 2008, 28(6):531-540
    [13] JIN J, CHEN Y, ZHANG S N, et al. A study of the pointed observation methods and sensitivity of HXMT[J]. Chin. Phys.:C, 2010, 34(1):66-71
    [14] NASA's HEASARC Software Packages[OL].[2014-03-11]. http://heasarc.gsfc.nasa.gov/docs/software.html
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  • 被引次数: 0
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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