Figure 2 from Estimating the Spin of the Black Hole Candidate MAXI J1659-152 with the X-Ray Continuum-fitting Method

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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 2.

The hardness−intensity diagram of MAXI J1659-152 from MAXI/GSC observations. The hardness is defined as the ratio of the counts detected at 4.0–10.0 keV to the counts detected at 2.0–4.0 keV of MAXI/GSC. The red circles above represent the observations by RXTE/PCA that we analyze in this paper, again with two points (SP2 and SP3) overlapping.

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