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Joint analysis of energy and RMS spectra from MAXI J1535-571 with Insight-HXMT

Authors :
Z. W. Li
Jin-Lu Qu
He Gao
Y. C. Zhu
Xin Lu
J. X. Wang
ShaoZhen Liu
S. Yang
Xufang Li
Z. Zhang
Z. L. Zhang
Gang Li
W. C. Zhang
Yan Zhu
Long Ji
N. Sai
F. Zhang
Wenda Zhang
Bin Meng
Y. Tan
W. C. Jiang
Chuan-Peng Zhang
He-Yang Liu
Guo-Ming Chen
ShiJie Zheng
Bobing Wu
Y. G. Zheng
C. Cai
J. F. Zhou
D. K. Zhou
T. Luo
Ti-Pei Li
Shuo Xiao
Yuan-Yuan Du
Zhe Chang
Y. N. Liu
X.W. Ma
Tianran Chen
Shu-Mei Jia
Yu-Dong Gu
Bo Lu
Mingyu Wu
Lian Tao
Bing Li
Xuchao Zhao
Jing Jin
Jia Huo
X. Y. Wen
Ju Guan
Fangjun Lu
Jundan Nie
Ge Ou
X. F. Li
Cheng-Cheng Guo
M. Gao
Lei Sun
Hongwei Liu
Y. G. Li
C. Z. Liu
Luhua Jiang
H. M. Zhang
C. Wang
W. S. Wang
W. Z. Zhang
W. G. Li
He Xu
G. H. Gao
Jin-Yuan Liao
X. L. Cao
Min-Xue Fu
Shaolin Xiong
Y. Nang
Y. S. Wang
Junqiang Zhang
Mingzhe Li
Jinyi Yang
Y. Zhang
C. K. Li
Y. Huang
GuoQing Liu
P. J. Wang
Youcai Zhang
Jing-Kang Deng
Xiaohua Liang
G. F. Wang
Yi Zhang
Yuan You
Youli Tuo
Xin Ren
Yin Xu
Weiguang Cui
Q. Luo
Qingcui Bu
L. D. Kong
Y. B. Chen
Ming-Yu Ge
Xiao-Jing Liu
Da-Wei Han
Shuang-Nan Zhang
Li-Ming Song
Wei-Wei Cui
Aimei Zhang
Shuinai Zhang
Peng Zhang
Y. W. Dong
G. C. Xiao
HongSheng Zhao
Y. P. Chen
Xiaobo Li
L. Chen
Yi-Yan Yang
X. Y. Song
Y. J. Yang
T. Zhang
Q. B. Yi
B. Y. Wu
Source :
Journal of High Energy Astrophysics. 25:29-38
Publication Year :
2020
Publisher :
Elsevier BV, 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.

Details

ISSN :
22144048
Volume :
25
Database :
OpenAIRE
Journal :
Journal of High Energy Astrophysics
Accession number :
edsair.doi...........d2b896083a2209238691d575df20e707