most citedA variable corona during the transition from type-C to type-B quasi-periodic oscillations in the black hole X-ray binary MAXI J1820+070

38 citations · 79 across the 5 of their papers we have counts for

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5 papers

astro-ph.HE2024

The bright black hole X-ray binary 4U 1543-47 during 2021 outburst. A clear state transition from super-Eddington to sub-Eddington accretion revealed by Insight-HXMT

Pei Jin, Guobao Zhang, Yuexin Zhang +9

We present a detailed analysis of the observations with the Hard X-ray Modulation Telescope of the black hole X-ray transient 4U~1543-47 during its outburst in 2021. We find a clea…

astro-ph.HE2023

Type-A quasi-periodic oscillation in the black hole transient MAXI J1348-630

Liang Zhang, Mariano Méndez, Federico García +12

We present a detailed analysis of the spectral and timing characteristics of a 7-Hz type-A quasi-periodic oscillation (QPO) detected in NICER observations of the black hole X-ray b…

astro-ph.HE202338 cited

A variable corona during the transition from type-C to type-B quasi-periodic oscillations in the black hole X-ray binary MAXI J1820+070

Ruican Ma, Mariano Mendez, Federico Garcia +3

We analyze a Neutron Star Interior Composition Explorer (NICER) observation of the black hole X-ray binary MAXI J1820+070 during a transition from type-C to type-B quasi-periodic o…

astro-ph.HE202316 cited

Fast transitions of X-ray variability in the black hole transient GX 339--4: comparison with MAXI J1820+070 and MAXI J1348-630

Zi-Xu Yang, Liang Zhang, S. N. Zhang +30

Fast transitions between different types of power density spectra (PDS) happening over timescales of several tens of seconds are rare phenomena in black hole X-ray binaries. In thi…

astro-ph.HE202325 cited

A NICER look at the jet-like corona of MAXI J1535-571 through type-B quasi-periodic oscillations

Yuexin Zhang, Mariano Méndez, Federico García +7

MAXI J1535-571 is a black-hole X-ray binary that in 2017 exhibited a very bright outburst which reached a peak flux of up to 5 Crab in the 2-20 keV band. Given the high flux, sever…