most citedHot disk of the Swift J0243.6+6124 revealed by Insight-HXMT

47 citations · 213 across the 13 of their papers we have counts for

collaborators

12 papers

astro-ph.HE202022 cited

Insight-HXMT firm detection of the highest energy fundamental cyclotron resonance scattering feature in the spectrum of GRO J1008-57

M. Y. Ge, L. Ji, S. N. Zhang +118

We report on the observation of the accreting pulsar GRO J1008-57 performed by Insight-HXMT at the peak of the source's 2017 outburst. Pulsations are detected with a spin period of…

astro-ph.HE20203 cited

Insight-HXMT insight into switch of the accretion mode: the case of the X-ray pulsar 4U 1901+03

Y. L. Tuo, L. Ji, S. S. Tsygankov +116

We use the In data collected during the 2019 outburst from X-ray pulsar 4U 1901+03 to complement the orbital parameters reported by Fermi/GBM. Using the Insight-HXMT, we examine th…

astro-ph.HE202034 cited

The evolution of the broadband temporal features observed in the black-hole transient MAXI J1820+070 with Insight-HXMT

Yanan Wang, Long Ji, S. N. Zhang +117

We study the evolution of the temporal properties of MAXI 1820+070 during the 2018 outburst in its hard state from MJD 58190 to 58289 with Insight-HXMT in a broad energy band 1-150…

astro-ph.HE2020

Joint Analysis of Energy and RMS Spectra from MAXI J1535-571 with Insight-HXMT

L. D. Kong, S. Zhang, Y. P. Chen +115

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-r…

astro-ph.HE2019

Diagnostic of the spectral properties of Aquila X-1 by Insight-HXMT snapshots during the early propeller phase

C. Güngör, M. Y. Ge, S. Zhang +108

We study the 2018 outburst of Aql X-1 via the monitor of all sky X-ray image (MAXI) data. We show that the outburst starting in February 2018 is a member of short-low class in the…

astro-ph.HE2019

-HXMT study of the timing properties of Sco X-1

S. M. Jia, Q. C. Bu, J. L. Qu +106

We present a detailed timing study of the brightest persistent X-ray source Sco X-1 using the data collected by the Hard X-ray Modulation Telescope (-HXMT) from July 2017…