A possible overall scenario for the outburst evolution of MAXI J1820+070 revealed by Insight-HXMT
J.Q.Peng, S.Zhang, Y.P.Chen, L.D.Kong, P.J.Wang, S.N.Zhang, L.Ji,, L.Tao, J.L.Qu, M.Y.Ge, Q.C.Shui, J.Li, Z.Chang, Z.S.Li, Y.X.Xiao

TL;DR
This study analyzes the spectral and timing evolution of MAXI J1820+070 during its 2018 outburst, revealing energy-dependent lags, changes in the corona, and a revised outburst hysteresis shape, providing insights into black hole accretion processes.
Contribution
It presents a detailed analysis of energy-dependent lags and corona evolution during the outburst, offering a new perspective on the outburst hysteresis shape in black hole transients.
Findings
Low-energy photons lag high-energy photons in the rise, opposite in decay.
The high-frequency break varies more in the hard X-ray band.
The corona coverage fraction changes significantly during the outburst.
Abstract
We study the spectral and temporal properties of the black hole X-ray transient binary MAXI J1820+070 during the 2018 outburst with Insight-HXMT observations. The outburst of MAXI J1820+070 can be divided into three intervals. For the two intervals of the outburst, we find that low-energy (below 140 keV) photos lag high-energy (140-170 keV) ones, while in the decay of the outburst, high-energy photons lag low-energy photons, both with a time scale of the order of days. Based on these results, the canonical hysteresis effect of the 'q' shape in the hardness-intensity diagram can be reformed into a roughly linear shape by taking into account the lag corrections between different energy bands. Time analysis shows that the high-frequency break of hard X-rays, derived from the power density spectrum of the first interval of the outburst is, in general, larger and more variable than that of…
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