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

Authors :
Kong, L.D.
Zhang, S.
Chen, Y.P.
Ji, L.
Zhang, S.N.
Yang, Y.R.
Tao, L.
Ma, X.
Qu, J.L.
Lu, F.J.
Bu, Q.C.
Chen, L.
Song, L.M.
Li, T.P.
Xu, Y.P.
Cao, X.L.
Chen, Y.
Liu, C.Z.
Cai, C.
Chang, Z.
Chen, G.
Chen, T.X.
Chen, Y.B.
Cui, W.
Cui, W.W.
Deng, J.K.
Dong, Y.W.
Du, Y.Y.
Fu, M.X.
Gao, G.H.
Gao, H.
Gao, M.
Ge, M.Y.
Gu, Y.D.
Guan, J.
Guo, C.C.
Han, D.W.
Huang, Y.
Huo, J.
Jia, S.M.
Jiang, L.H.
Jiang, W.C.
Jin, J.
Li, 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.
Liang, X.H.
Liao, J.Y.
Liu, G.Q.
Liu, H.X.
Liu, H.W.
Liu, S.Z.
Liu, X.J.
Liu, Y.N.
Lu, B.
Lu, X.F.
Luo, Q.
Luo, T.
Meng, B.
Nang, Y.
Nie, J.Y.
Ou, G.
Ren, X.Q.
Sai, N.
Song, X.Y.
Sun, L.
Tan, Y.
Tuo, Y.L.
Wang, C.
Wang, G.F.
Wang, J.
Wang, P.J.
Wang, W.S.
Wang, Y.S.
Wen, X.Y.
Wu, B.Y.
Wu, B.B.
Wu, M.
Xiao, G.C.
Xiao, S.
Xiong, S.L.
Xu, H.
Yang, J.W.
Yang, S.
Yang, Y.J.
Yi, Q.B.
You, Y.
Zhang, 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.
Zhao, H.S.
Zhao, X.F.
Zheng, S.J.
Zheng, Y.G.
Zhou, D.K.
Zhou, J.F.
Zhu, Y.X.
Zhu, Y.
Source :
Journal of High Energy Astrophysics; March 2020, Vol. 25 Issue: 1 p29-38, 10p
Publication Year :
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

Language :
English
ISSN :
22144048
Volume :
25
Issue :
1
Database :
Supplemental Index
Journal :
Journal of High Energy Astrophysics
Publication Type :
Periodical
Accession number :
ejs52164763
Full Text :
https://doi.org/10.1016/j.jheap.2020.01.003