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A Parametric Model to Reproduce the Background of the Insight-HXMT/HE Blind Detector

  • Authors: Yuan You, Jin-Yuan Liao, Shuang-Nan Zhang, Shu Zhang, Xue-Feng Lu, Juan Zhang, Gang Li, Zhi Chang, Yu-Peng Chen, Ming-Yu Ge, Cheng-Cheng Guo, Rui Huang, Yue Huang, Jing Jin, Xiao-Bo Li, Xu-Fang Li, Zheng-Wei Li, Cong-Zhan Liu, Fang-Jun Lu, Jian-Yin Nie, Li-Ming Song, Si-Fan Wang, Yi-Fei Zhang, Hai-Sheng Zhao

Yuan You et al 2021 The Astrophysical Journal Supplement Series 256 .

  • Provider: AAS Journals

Caption: Figure 4.

Count rate map of HBD at 28–334 keV for ascending (top) and descending (bottom) orbital directions; the white region is the SAA, where all HEDs shut down for instrument protection. The difference between the two maps is mainly caused by the delayed background activated in the SAA.

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