activity
20052026
most citedDiscovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMT

129 citations · 479 across the 31 of their papers we have counts for

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16 papers · 1 filter

astro-ph.HE2025★ 18 cited

PSR J1231-1411 revisited: Pulse Profile Analysis of X-ray Observation

Liqiang Qi, Shijie Zheng, Juan Zhang +14

One of the primary goals of Neutron Star Interior Composition Explorer (NICER)-like X-ray missions is to impose stringent constraints on the neutron star equation of state by preci…

astro-ph.HE2023★ 16 cited

Hilbert-Huang Transform analysis of quasi-periodic oscillations in MAXI J1820+070

Wei Yu, Qing-Cui Bu, Zi-Xu Yang +14

We present time-frequency analysis, based on the Hilbert-Huang transform (HHT), of the evolution on the low-frequency quasi-periodic oscillations (LFQPOs) observed in the black hol…

astro-ph.HE2023

A spectral-timing study of the inner flow geometry in MAXI J1535--571 with -HXMT and NICER

Wei Yu, Qing-Cui Bu, He-Xin Liu +48

We have performed a spectral-timing analysis on the black hole X-ray binary MAXI J1535--571 during its 2017 outburst, with the aim of exploring the evolution of the inner accretion…

astro-ph.HE2023★ 43 cited

Synchrotron Radiation Dominates the Extremely Bright GRB 221009A

Jun Yang, Xiao-Hong Zhao, Zhenyu Yan +30

The brightest Gamma-ray burst, GRB 221009A, has spurred numerous theoretical investigations, with particular attention paid to the origins of ultra-high energy TeV photons during t…

astro-ph.HE2023★ 33 cited

Insight-HXMT and GECAM-C observations of the brightest-of-all-time GRB 221009A

Zheng-Hua An, S. Antier, Xing-Zi Bi +174

GRB 221009A is the brightest gamma-ray burst ever detected since the discovery of this kind of energetic explosions. However, an accurate measurement of the prompt emission propert…

astro-ph.HE2023★ 2 cited

Atlas of dynamic spectra of fast radio burst FRB 20201124A

Bo-Jun Wang, Heng Xu, Jin-Chen Jiang +64

Fast radio bursts (FRBs) are highly dispersed millisecond-duration radio bursts, of which the physical origin is still not fully understood. FRB 20201124A is one of the most active…

astro-ph.HE2022★ 11 cited

Determination of QPO properties in the presence of strong broad-band noise: a case study on the data of MAXI J1820+070

Deng-Ke Zhou, Shuang-Nan Zhang, Li-Ming Song +8

Accurate calculation of the phase lags of quasi-periodic oscillations (QPOs) will provide insight into their origin. In this paper we investigate the phase lag correction method wh…

astro-ph.HE2022★ 26 cited

Revisit the periodicity of SGR J1935+2154 bursts with updated sample

Sheng-Lun Xie, Ce Cai, Shao-Lin Xiong +30

Since FRB 200428 has been found to be associated with an X-ray burst from the Galactic magnetar SGR J1935+2154, it is interesting to explore whether the magnetar bursts also follow…

astro-ph.HE2022★ 36 cited

The Peculiar Precursor of a Gamma-Ray Burst from a Binary Merger Involving a Magnetar

Shuo Xiao, Yan-Qiu Zhang, Zi-Pei Zhu +42

The milestone discovery of GW 170817-GRB 170817A-AT 2017gfo has shown that gravitational wave (GW) could be produced during the merger of neutron star-neutron star/black hole and t…

astro-ph.HE2022★ 5 cited

GRB 210121A: Observation of photospheric emissions from different regimes and the evolution of the outflow

Xin-Ying Song, Shuang-Nan Zhang, Shu Zhang +2

GRB 210121A was observed by Insight-HXMT, Gravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM), Fermi Gamma-ray Burst Monitor (Fermi/GBM) on Jan 21st…

astro-ph.HE2022★ 22 cited

The First Insight-HXMT Gamma-Ray Burst Catalog: The First Four Years

Xin-Ying Song, Shao-Lin Xiong, Shuang-Nan Zhang +40

The Hard X-ray Modulation Telescope (Insight-HXMT), is China's first X-ray astronomy satellite launched on June 15, 2017. The anti-coincidence CsI detectors of the High Energy X-ra…

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.HE2019★ 7 cited

A peculiar cyclotron line near 16 keV detected in the 2015 outburst of 4U 0115+63?

Bai-Sheng Liu, Lian Tao, Shuang-Nan Zhang +8

In 2015 October, the Be/X-ray binary 4U 0115+63 underwent a type II outburst, reaching an X-ray luminosity of {\DP{38}\es}. During the outburst, Nuclear Spectroscopic Telesc…

astro-ph.HE2019★ 16 cited

Statistical properties of the repeating fast radio burst source FRB 121102

Bing Li, Long-Biao Li, Zhi-Bin Zhang +4

Currently, FRB 121102 is the only fast radio burst source that was observed to give out bursts repeatedly. It shows a high repeating rate, with more than one hundred bursts being s…

astro-ph.HE2018★ 19 cited

Probing Magnetic Fields of GRB X-ray Flares with Polarization Observations

Jin-Jun Geng, Yong-Feng Huang, Xue-Feng Wu +2

X-ray flares, lasting for s in the X-ray band, are often observed following gamma-ray bursts (GRBs). The physical origin of X-ray flares is still unknown merely w…

astro-ph.HE2018★ 16 cited

Continued Brightening of the Afterglow of GW170817/GRB 170817A as due to a Delayed Energy Injection

Bing Li, Long-Biao Li, Yong-Feng Huang +3

The brightness of the multi-wavelength afterglow of GRB 170817A is increasing unexpectedly even 160 days after the associated gravitational burst. Here we suggest that the b…