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25 April 2024

» arxiv » 2001.6637

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Joint Analysis of Energy and RMS Spectra from MAXI J1535-571 with Insight-HXMT
L. D. Kong ; S. Zhang ; Y. P. Chen ; L. Ji ; S. N. Zhang ; Y. R. Yang ; L. Tao ; X. Ma ; J. L. Qu ; F. J. Lu ; Q. C. Bu ; L. Chen ; L. M. Song ; T. P. Li ; Y. P. Xu ; X. L. Cao ; Y. Chen ; C. Z. Liu ; C. Cai ; Z. Chang ; G. Chen ; T. X. Chen ; Y. B. Chen ; W. Cui ; W. W. Cui ; J. K. Deng ; Y. W. Dong ; Y. Y. Du ; M. X. Fu ; G. H. Gao ; H. Gao ; M. Gao ; M. Y. Ge ; Y. D. Gu ; J. Guan ; C. C. Guo ; D. W. Han ; Y. Huang ; J. Huo ; S. M. Jia ; L. H. Jiang ; W. C. Jiang ; J. Jin ; B. Li ; C. K. Li ; G. Li ; M. S. Li ; W. Li ; X. Li ; X. B. Li ; X. F. Li ; Y. G. Li ; Z. W. Li ; X. H. Liang ; J. Y. Liao ; G. Q. Liu ; H. X. Liu ; H. W. Liu ; S. Z. Liu ; X. J. Liu ; Y. N. Liu ; B. Lu ; X. F. Lu ; Q. Luo ; T. Luo ; B. Meng ; Y. Nang ; J. Y. Nie ; G. Ou ; X. Q. Ren ; N. Sai ; X. Y. Song ; L. Sun ; Y. Tan ; Y. L. Tuo ; C. Wang ; G. F. Wang ; J. Wang ; P. J. Wang ; W. S. Wang ; Y. S. Wang ; X. Y. Wen ; B. Y. Wu ; B. B. Wu ; M. Wu ; G. C. Xiao ; S. Xiao ; S. L. Xiong ; H. Xu ; J. W. Yang ; S. Yang ; Y. J. Yang ; Q. B. Yi ; Y. You ; A. M. Zhang ; C. M. Zhang ; F. Zhang ; H. M. Zhang ; J. Zhang ; P. Zhang ; T. Zhang ; W. Zhang ; W. C. Zhang ; W. Z. Zhang ; Y. Zhang ; Y. F. Zhang ; Y. J. Zhang ; Y. H. Zhang ; Y. Zhang ; Z. Zhang ; Z. L. Zhang ; H. S. Zhao ; X. F. Zhao ; S. J. Zheng ; Y. G. Zheng ; D. K. Zhou ; J. F. Zhou ; Y. X. Zhu ; Y. Zhu ;
Date:	18 Jan 2020
Abstract:	A new black hole X-ray binary (BHXRB) MAXI J1535-571 was discovered by MAXI during its outburst in 2017. Using observations taken by the first Chinese X-ray satellite, the Hard X-ray Modulation Telescope (dubbed as Insight-HXMT), we perform a joint spectral analysis (2-150 keV) in both energy and time domains. The energy spectra provide the essential input for probing the intrinsic Quasi-Periodic Oscillation (QPO) fractional rms spectra (FRS). Our results show that during the intermediate state, the energy spectra are in general consistent with those reported by Swift/XRT and NuSTAR. However, the QPO FRS become harder and the FRS residuals may suggest the presence of either an additional power-law component in the energy spectrum or a turn-over in the intrinsic QPO FRS at high energies.
Source:	arXiv, 2001.6637
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