1. spin of new black hole candidate: MAXI J1803−298 observed by NuSTAR and NICER.
- Author
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Feng, Ye, Zhao, Xueshan, Li, Yufeng, Gou, Lijun, Jia, Nan, Liao, Zhenxuan, and Wang, Yuan
- Subjects
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BLACK holes , *X-ray reflection , *EXTREME value theory , *ACCRETION disks , *CONFIDENCE intervals - Abstract
MAXI J1803−298, a newly-discovered Galactic transient, and black hole candidate was first detected by MAXI /GSC on 2021 May 01. In this paper, we present a detailed spectral analysis of MAXI J1803−298. Utilizing the X-ray reflection fitting method, we perform a joint fit to the spectra of MAXI J1803−298, respectively, observed by NuSTAR and NICER /XTI on the same day over the energy range between 0.7–79.0 keV in SIMS state, and the observed inner radius of the accretion disc is demonstrated to have extended to the ISCO radius (R in =1.08 R ISCO). Implementing the relativistic reflection model relxillCp , we found its spin (and the inclination angle i) can be constrained to be close to an extreme value, 0.991 (i ∼ 70 °), at 68 per cent confidence interval. The results suggest that MAXI J1803−298 may be a fast-rotating black hole with a large inclination angle. [ABSTRACT FROM AUTHOR]
- Published
- 2022
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