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Status of the Hard X-ray Modulation Telescope (Insight-HXMT) Project

LU Fangjun ZHANG Shuangnan

LU Fangjun, ZHANG Shuangnan. Status of the Hard X-ray Modulation Telescope (Insight-HXMT) Project[J]. 空间科学学报, 2018, 38(5): 623-626. doi: 10.11728/cjss2018.05.623
引用本文: LU Fangjun, ZHANG Shuangnan. Status of the Hard X-ray Modulation Telescope (Insight-HXMT) Project[J]. 空间科学学报, 2018, 38(5): 623-626. doi: 10.11728/cjss2018.05.623
LU Fangjun, ZHANG Shuangnan. Status of the Hard X-ray Modulation Telescope (Insight-HXMT) Project[J]. Chinese Journal of Space Science, 2018, 38(5): 623-626. doi: 10.11728/cjss2018.05.623
Citation: LU Fangjun, ZHANG Shuangnan. Status of the Hard X-ray Modulation Telescope (Insight-HXMT) Project[J]. Chinese Journal of Space Science, 2018, 38(5): 623-626. doi: 10.11728/cjss2018.05.623

Status of the Hard X-ray Modulation Telescope (Insight-HXMT) Project

doi: 10.11728/cjss2018.05.623
基金项目: 

Supported by the Major Program of the National Natural Science Foundation of China (41590851)

详细信息
    作者简介:

    LU Fangjun,lufj@ihep.ac.cn;ZHANG Shuangnan,zhangsn@ihep.ac.cn

Status of the Hard X-ray Modulation Telescope (Insight-HXMT) Project

Funds: 

Supported by the Major Program of the National Natural Science Foundation of China (41590851)

More Information
    Author Bio:

    LU Fangjun,lufj@ihep.ac.cn;ZHANG Shuangnan,zhangsn@ihep.ac.cn

  • 摘要: The Hard X-ray Modulation Telescope (HXMT) was launched at Jiuquan Satellite Launch Center on June 15, 2017, and was named as Insight-HXMT after the launch. Now all the instruments work properly in space, dozens of sources have been observed, and some early scientific results have been published. The nominal lifetime of Insight-HXMT is 4 years.

     

  • [1] LI T P. Science with the hard X-ray modulation telescope[J]. Int. J. Mod. Phys.:D, 2013, 22:1360005
    [2] LU F J. The Hard X-ray Modulation Telescope (HXMT):mission and its current status[J]. Assoc. Asia Pacific Phys. Soc. Bull., 2009, 29(2):36
    [3] LU F J. Status of the hard X-ray modulation telescope project[J]. Chin. J. Space Sci., 2014, 34(5):544
    [4] ZHANG S, LU F J, ZHANG S N, et al. Introduction to Fig. 7 Low frequency QPOs detected by HE (a), ME (b) and LE (c) under an exposure of 3 ks, during the low/hard state of the outburst from the BH candidate MAXI J1535-571. The dotted blue lines represent the various components used to fit the power-density spectrum, and the solid red line is the sum of these components the hard X-ray modulation telescope[J]. SPIE, 2014, 9144E:21
    [5] ZHANG S, ZHANG S N, LU F J, et al. The insightHXMT mission and its recent progresses[J]. SPIE, 2018(submitted)
    [6] LI X B, SONG L M, LI X F, et al. In-orbit calibration status of the insight-HXMT[J]. SPIE, 2018(submitted)
    [7] YANG X J, LU F J, CHEN L. High spatial resolution X-ray spectroscopy of Cas A with Chandra[J]. Chin. J. Astron. Astrophys., 2008, 8:439-450
    [8] ABBOTT B P, ABBOTT R, ABBOTT T D, et al. Multimessenger observation of a binary neutron star merger[J]. Astrophys. J., 2017, 848:L12
    [9] LI T P, XIONG S L, ZHANG S N, et al. Sciences China physics[J]. Mech. Astron., 2017, 61(3):1011
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出版历程
  • 收稿日期:  2018-06-03
  • 刊出日期:  2018-09-15

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