activity
20232025
most citedA Phase-resolved View of the Low-frequency Quasiperiodic Oscillations from the Black Hole Binary MAXI J1820+070

19 citations · 43 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2025★ 6 cited

A polarized view of the young Pulsar Wind Nebula 3C 58 with IXPE

N. Bucciantini, J. Wong, R. W. Romani +11

Pulsar Wind nebulae (PWNe), are among the most efficient particle accelerators in the Universe, however understanding the physical conditions and the magnetic geometry in their inn…

astro-ph.HE2024

A multi-band study of pulsar glitches with Fermi-LAT and Parkes

P. Liu, J. -P. Yuan, M. -Y. Ge +10

Pulsar glitch is a phenomenon characterized by abrupt changes in the spin period over less than a minute. We present a comprehensive analysis of glitches in four gamma-ray pulsars…

astro-ph.HE2024

Broadband noise and quasi-periodic oscillation characteristics of the X-ray pulsar RX J0440.9+4431

P. P. Li, L. Tao, R. C. Ma +15

We present a comprehensive timing analysis on the Be/X-ray binary pulsar RX J0440.9+4431 using observations from \textit{NICER} and \textit{Insight}-HXMT during the 2022--2023 outb…

astro-ph.HE2024

Pulsed Iron line Emission from the First Galactic Ultraluminous X-ray Pulsar Swift J0243.6+6124

Y. X. Xiao, Y. J. Xu, M. Y. Ge +14

We report the phase-resolved spectral results of the first Galactic Pulsating Ultra-Luminous X-ray source (PULX) Swift J0243.6+6124, modeling at its 2017-2018 outburst peak using d…

astro-ph.HE2023★ 11 cited

Pulse profile variability associated with the glitch of PSR J10485832

P. Liu, J. -P. Yuan, M. -Y. Ge +10

PSR J10485832 (B104658) is a Vela-like pulsar that has exhibited multiple glitch events. In this study, we analyze the timing data spanning nearly 16 years, acquired from bot…

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★ 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…