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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, and Hai-Sheng Zhao

2021 The Astrophysical Journal Supplement Series 256 47.

  • Provider: AAS Journals

Caption: Figure 11.

Satellite tracks of one group of light curves in the world map. The red lines are a group of light curves of 4.5 ks; their tracks are almost the same with a difference <4°. The green line is the border of the SAA. To fit the delayed background of this group of light curves, data in the most recent 100 ks are selected as the input data of the parametric model, drawn as blue lines. The data of the coastline in the background of this figure are provided by the ETOPO1 Global Relief Model of NOAA (Amante & Eakins 2009).

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