collaborators

10 papers

astro-ph.HE2026

Phase-resolved QPO Analysis of GX 339-4: Improved Technique and Consistent Behaviors between QPOs and Broadband Noise

Jin Qin, Hua Feng, Liang Zhang +5

The nature of low-frequency quasi-periodic oscillations (QPOs) in black hole X-ray binaries remains unclear, and their relationship with the accompanying broadband noise (BBN) is s…

astro-ph.HE2026

An Insight-HXMT View of the Evolution of the Type-C Quasiperiodic Oscillation during the Flaring State of Swift J1727.8-1613

Min Wei, Xiang Ma, Liang Zhang +16

We present a detailed analysis of the evolution of type-C quasiperiodic oscillations (QPOs) observed during the flaring state of the recently discovered black hole X-ray binary Swi…

astro-ph.IM2026

A New Method for Identifying Contaminating Sources and Locating Target Sources through the Cross-Arm Features of Micro Pore Optics

Yiming Huang, Lian Tao, Jin-Yuan Liao +15

The Pathfinder of the Type-A satellites in the Chasing All Transients Constellation Hunters (CATCH) space mission is equipped with Micro-Pore Optics (MPOs) and four single-pixel Si…

astro-ph.HE2026

Discovery of energy-dependent phase variations in the polarization angle of Cen X-3

Qing-Chang Zhao, Lian Tao, Sergey S. Tsygankov +7

We present a detailed polarimetric analysis of Cen X-3 using \ixpe observations during its high state, revealing complex energy-dependent polarization behavior. While phase-average…

astro-ph.HE2026

X-ray and radio observations of the AMXP MAXI J1957+032 covering the 2022-2025 outbursts

Zhaosheng Li, Lucien Kuiper, Yuanyue Pan +12

We presented a comprehensive multi-epoch timing and multiwavelength analysis of the accreting millisecond X-ray pulsar MAXI J1957+032, covering two major outbursts in 2022 and 2025…

astro-ph.HE2026

Characteristics of the High-frequency Humps in the Black hole X-ray Binary Swift J1727.8--1613

Ze-Xi Li, Liang Zhang, Lian Tao +13

We present a detailed timing analysis of the two high-frequency humps observed in the power density spectrum of Swift J1727.8--1613 up to 100 keV, using data from the Hard X-ray Mo…