activity
20202024
most citedHXMT Identification of a non-thermal X-ray burst from SGR J1935+2154 and with FRB 200428

274 citations · 836 across the 28 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.HE2020★ 17 cited

Insight-HXMT observations of a possible fast transition from jet to wind dominated state during a huge flare of GRS~1915+105

L. D. Kong, S. Zhang, Y. P. Chen +92

We present the analysis of the brightest flare that was recorded in the \emph{Insight}-HMXT data set, in a broad energy range (2200 keV) from the microquasar GRS~1915+105 during…

astro-ph.HE2020★ 51 cited

Estimating the black hole spin for the X-ray binary MAXI J1820+070

Xueshan Zhao, Lijun Gou, Yanting Dong +6

MAXI J1820+070 is a newly-discovered black hole X-ray binary, whose dynamical parameters, namely the black hole mass, the inclination angle and the source distance, have been estim…

astro-ph.HE2020★ 129 cited

Discovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMT

Xiang Ma, Lian Tao, Shuang-Nan Zhang +119

Low-frequency quasi-periodic oscillations (LFQPOs) are commonly found in black hole X-ray binaries, and their origin is still under debate. The properties of LFQPOs at high energie…

astro-ph.HE2020★ 18 cited

Discovery of state transition behaviors in PSR J1124--5916

M. Y. Ge, J. P. Yuan, F. J. Lu +7

With the twelve-year long observations by {\sl Fermi}-LAT, we discover two pairs of spin-down state transitions of PSR J1124--5916, making it the second young pulsar detected to ha…

astro-ph.HE2020★ 274 cited

HXMT Identification of a non-thermal X-ray burst from SGR J1935+2154 and with FRB 200428

C. K. Li, L. Lin, S. L. Xiong +117

Fast radio bursts (FRBs) are short pulses observed in radio band from cosmological distances. One class of models invoke soft gamma-ray repeaters (SGRs), or magnetars, as the sourc…

astro-ph.HE2020★ 3 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…