activity
20002023
most citedInsight-HXMT observations of the New Black Hole Candidate MAXI J1535-571: timing analysis

99 citations · 444 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2023★ 1 cited

Change of rotation measure during eclipse of a black widow PSR J20510827

S. Q. Wang, J. B. Wang, D. Z. Li +15

Black widows are millisecond pulsars ablating their companions. The material blown from the companion blocks the radio emission, resulting in radio eclipses. The properties of the…

astro-ph.HE2022★ 11 cited

Study on the magnetic field strength of NGC 300 ULX1

Y. Y. Pan, Z. S. Li, C. M. Zhang +1

NGC 300 ULX1 is a pulsating ultraluminous X-ray source (PULX) with the longest spin period of and a high spin-up rate of $\dot P\simeq5.56\times10^{-7}\,\rm s\…

astro-ph.HE2021★ 14 cited

A broadband radio study of PSR J0250+5854: the slowest-spinning radio pulsar known

C. H. Agar, P. Weltevrede, L. Bondonneau +19

We present radio observations of the most slowly rotating known radio pulsar PSR J0250+5854. With a 23.5 s period, it is close, or even beyond, the - diagram region tho…

astro-ph.HE2020★ 14 cited

Insight-HXMT observations of Swift J0243.6+6124: the evolution of RMS pulse fractions at super-Eddington luminosity

P. J. Wang, L. D. Kong, S. Zhang +116

Based on Insight-HXMT data, we report on the pulse fraction evolution during the 2017-2018 outburst of the newly discovered first Galactic ultraluminous X-ray source (ULX) Swift J0…

astro-ph.HE2020★ 19 cited

Discovery of delayed spin-up behavior following two large glitches in the Crab pulsar, and the statistics of such processes

M. Y. Ge, S. N. Zhang, F. J. Lu +130

Glitches correspond to sudden jumps of rotation frequency () and its derivative () of pulsars, the origin of which remains not well understood yet, partly because the jum…

astro-ph.HE2020★ 30 cited

A search for prompt gamma-ray counterparts to fast radio bursts in the Insight-HXMT data

C. Guidorzi, M. Marongiu, R. Martone +118

No robust detection of prompt electromagnetic counterparts to fast radio bursts (FRBs) has yet been obtained, in spite of several multi-wavelength searches carried out so far. Spec…