activity
20102025
most citedOverview to the Hard X-ray Modulation Telescope (Insight-HXMT) Satellite

329 citations · 2.6k across the 96 of their papers we have counts for

collaborators

96 papers

astro-ph.HE2025★ 3 cited

New insight into the hard X-ray emission influenced by the type-\uppercase\expandafter{\romannumeral1} bursts observed by Insight-HXMT during outburst of 4U 1636--536

J. Q. Peng, S. Zhang, Y. P. Chen +17

By analyzing the data from Insight-HXMT and NICER, we can determine the evolution of the significance of the hard shortage in 4U 1636--536 with its spectral state, as well as the e…

astro-ph.HE2025★ 9 cited

Back to business: SLX 1746--331 after 13 years of silence

Jing-Qiang Peng, Shu Zhang, Peng-Ju Wang +17

The black hole candidate system SLX 1746--331 was back to business in 2023, after a long silence of roughly 13 years. An outburst was observed thoroughly by \textit{Insight}-HXMT a…

astro-ph.HE2025★ 4 cited

Insight-HXMT observations on thermonuclear X-ray bursts from 4U~1608--52 in the low/hard state: the energy-dependant hard X-ray deficit and cooling saturation of the corona

Y. P. Chen, S. Zhang, L. Ji +9

During thermonuclear bursts, it is suspected that {\bf the cooling of the corona by the burst emission} may be the cause of hard X-ray {\bf deficits}. Although this {\bf deficit} h…

astro-ph.HE2025★ 4 cited

New insight into the Rapid Burster by Insight-HXMT

Y. P. Chen, S. Zhang, S. N. Zhang +91

We report the timing and spectral analyses upon of the type II X-ray bursts from the Rapid Burster (MXB 1730--335) observed by Insight-HXMT and Swift/XRT. By stacking the long-dura…

astro-ph.HE2024

estimating the spin of MAXI J1348--630 from intermediate and soft states using \textit{Insight}-HXMT data

J. Guan, R. C. Ma, L. Tao +6

We present a broadband spectral analysis of the soft-intermediate and soft states using \textit{Insight}-HXMT observations of the black hole binary MAXI J1348--630 during its outbu…

astro-ph.HE2024

A Revised Spin of the Black Hole in GRS 1716-249 with a New Distance

S. J. Zhao, L. Tao, Q. Q. Yin +12

GRS 1716-249 is a stellar-mass black hole in a low-mass X-ray binary that underwent a gaint outburst in 2016/17. In this paper we use simultaneous observations of Insight-HXMT and…

astro-ph.HE2023★ 19 cited

A Phase-resolved View of the Low-frequency Quasiperiodic Oscillations from the Black Hole Binary MAXI J1820+070

Qing C. Shui, S. Zhang, Shuang N. Zhang +21

Although low-frequency quasiperiodic oscillations (LFQPOs) are commonly detected in the X-ray light curves of accreting black hole X-ray binaries, their origin still remains elusiv…

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.HE2023★ 7 cited

Detection of a strong ~2.5 Hz modulation in the Newly Discovered Millisecond Pulsar MAXI J1816-195

P. P. Li, L. Tao, L. Zhang +16

MAXI J181-195 is a newly discovered accreting millisecond X-ray pulsar that went outburst in June 2022. Through timing analysis with NICER and NuSTAR observations, we find a transi…

astro-ph.HE2023★ 12 cited

Spin measurement of 4U 1543-47 with Insight-HXMT and NICER from its 2021 outburst: A test of accretion disk models at high luminosities

E. S. Yorgancioglu, Q. C. Bu, A. Santangelo +7

4U 1543--47 is one of a handful of known black hole candidates located in the Milky Way Galaxy, and has undergone a very bright outburst in 2021, reaching a total of 9 Crab,…

astro-ph.HE2023★ 2 cited

The mHz quasi-regular modulations of 4U 1630--47 during its 1998 outburst

Qingchang Zhao, Hongxing Yin, Lian Tao +19

We present the results of a detailed timing and spectral analysis of the quasi-regular modulation (QRM) phenomenon in the black hole X-ray binary 4U 1630--47 during its 1998 outbur…

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.IM2023★ 5 cited

In-orbit background simulation of a type-B CATCH satellite

Jingyu Xiao, Liqiang Qi, Shuang-Nan Zhang +23

The Chasing All Transients Constellation Hunters (CATCH) space mission plans to launch three types of micro-satellites (A, B, and C). The type-B CATCH satellites are dedicated to l…

astro-ph.HE2023★ 9 cited

X-ray Polarimetry of the accreting pulsar 1A~0535+262 in the supercritical state with PolarLight

Xiangyun Long, Hua Feng, Hong Li +25

The X-ray pulsar 1A 0535+262 exhibited a giant outburst in 2020, offering us a unique opportunity for X-ray polarimetry of an accreting pulsar in the supercritical state. Measureme…

astro-ph.HE2023★ 16 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.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★ 24 cited

A detailed view of low-frequency quasi-periodic oscillation in the broadband 0.2-200 keV with Insight-HXMT and NICER

X. Ma, L. Zhang, L. Tao +13

We report the X-ray timing results of the black hole candidate MAXI J1820+070 during its 2018 outburst using the Hard X-ray Modulation Telescope (Insight-HXMT) and Neutron Star Int…

astro-ph.HE2022★ 12 cited

Trace the Accretion Geometry of H 1743--322 with Type C Quasi-periodic Oscillations in Multiple Outbursts

Qing-Cang Shui, Shu Zhang, Yu-Peng P. Chen +12

We present a systematic analysis of type C quasi-periodic oscillation (QPO) observations of H 1743--322 throughout the Rossi X-ray Timing Explorer (RXTE) era. We find that, while d…

astro-ph.IM2022★ 24 cited

CATCH: Chasing All Transients Constellation Hunters Space Mission

Panping Li, Qian-Qing Yin, Zhengwei Li +34

In time-domain astronomy, a substantial number of transients will be discovered by multi-wavelength and multi-messenger observatories, posing a great challenge for follow-up capabi…

astro-ph.HE2022★ 1 cited

Monte-Carlo simulations on possible collimation effects of outflows to fan-beamed emission of ultraluminous accreting X-ray pulsars

X. Hou, Y. You, L. Ji +10

Pulsating ultraluminous X-ray sources (PULXs) are accreting pulsars with apparent X-ray luminosity exceeding . We perform Monte-Carlo simulations to inve…

astro-ph.HE2022★ 5 cited

Return of 4U~1730--22 after 49 years silence: the spectral properties of the 2021/2022 outbursts observed by NICER and Insight-HXMT and the soft-to-hard state transition caused by the propeller effect

Yu-Peng Chen, Shu Zhang, Shuang-Nan Zhang +10

After in quiescence for 49 years, 4U~1730--22 became active and had two outbursts in 2021 \& 2022, the onset and tail of the outbursts were observed by NICER, which give us a peerl…

astro-ph.HE2022★ 16 cited

A possible 250-second X-ray quasi-periodicity in the fast blue optical transient AT2018cow

Wenjie Zhang, Xinwen Shu, Jin-Hong Chen +11

The fast blue optical transients (FBOTs) are a new population of extragalactic transients of unclear physical origin. A variety of mechanisms have been proposed including failed su…

astro-ph.HE2022★ 4 cited

Return of 4U~1730--22 after 49 years silence: the peculiar burst properties of the 2021/2022 outbursts observed by Insight-HXMT

Yu-Peng Chen, Shu Zhang, Long Ji +10

After in quiescence for 49 years, 4U~1730--22 became active and had two outbursts in 2021 \& 2022; ten thermonuclear X-ray bursts were detected with Insight-HXMT. Among them, the f…