collaborators

23 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

First Gamma-Ray Burst Observations with SVOM

F. Daigne, D. Turpin, J. -L. Atteia +34

Following its launch on 22 June 2024, the Space-based multi-band astronomical Variable Objects Monitor (SVOM) successfully completed its flight acceptance, commissioning, and scien…

astro-ph.HE2026

Rapid quasi-periodic reconfiguration of the accretion column in pulsar 1A 0535+262

Lingda Kong, Xiaohang Dai, Andrea Santangelo +12

Accretion onto strongly magnetized neutron stars is commonly interpreted using quasi-steady models, in which the accretion-column structure adjusts smoothly to the mass inflow rate…

astro-ph.HE2026

Discovery of Short-Term γ-Ray Pulsed Radiation Variations Following a Glitch in PSR J0205+6449

Wen-Tao Ye, Ming-Yu Ge, Shi-Jie Zheng +7

Rotation-powered pulsars exhibit stable emission characteristics most of the time. However, their radiative state can vary with the sudden changes of rotational state such as glitc…

astro-ph.HE2026

Search for the Highest-energy Quasiperiodic Oscillation in the Black Hole X-Ray Binary Candidate Swift J1727.8-1613

Xiang Ma, Qing-Cang Shui, Ming-Yu Ge +8

We report the first detection of a low-frequency quasiperiodic oscillation (QPO) extending above 250 keV in the black hole X-ray binary candidate Swift J1727.8-1613 using Insight-H…

astro-ph.HE2026

Multiwavelength Analysis of PSR J0437-4715 with Pulse Profile Modeling

Liqiang Qi, Juan Zhang, Weiwei Xu +6

We present a multi-wavelength analysis of the nearby millisecond pulsar PSR J0437--4715, combining Hubble Space Telescope (HST) far-ultraviolet, ROSAT soft X-ray, and XMM-Newton X-…