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Estimating the Spin of the Black Hole Candidate MAXI J1659-152 with the X-Ray Continuum-fitting Method

  • Authors: Ye Feng, Xueshan Zhao, Lijun Gou, Jianfeng Wu, James F. Steiner, Yufeng Li, Zhenxuan Liao, Nan Jia, and Yuan Wang

2022 The Astrophysical Journal 925 142.

  • Provider: AAS Journals

Caption: Figure 1.

The light curve of MAXI J1659-152 over the past 11 yr as observed by MAXI/GSC. The inset shows the evolution of the hardness ratio during the 2010 outburst. The hardness is defined as the ratio of the counts detected at 4.0–10.0 keV (hard X-ray bands) to the counts detected at 2.0–4.0 keV (soft X-ray bands) of MAXI/GSC. The red circles in inset correspond to dates with observations by RXTE/PCA, with two points (SP2 and SP3) overlapping.

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