most citedGRB Timing: Decoding the Hidden Slow Jets in GRB 060729

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astro-ph.HE2026

Constraints on the Low-frequency Radio Emission of the Galactic FRB Source SGR 1935+2154

Chen-Ran Hu, Jinhuang Cao, S. A. Tyul'bashev +13

We present a search for radio pulses from the Galactic magnetar SGR 1935+2154, a well-known source of fast radio bursts (FRBs), at 110 MHz using the Large Phased Array (LPA)…

astro-ph.HE2026

Are Repeaters Prevalent Among the Known Fast Radio Burst Sources?

Xiao-Fei Dong, Qing Pan, Yong-Feng Huang +10

Fast radio bursts (FRBs) are millisecond radio pulses of unknown origin. Despite extensive follow-up observations, only of FRBs have been confirmed as repeaters. It remai…

astro-ph.HE2026

Diverse Morphologies of GRB X-Ray Plateaus within a Common Magnetar Framework

Xiao-Fei Dong, Yong-Feng Huang, Nurimangul Nurmamat +7

The origin of the X-ray plateau phase in gamma-ray bursts (GRBs) remains an open problem. In particular, it is unclear whether GRBs with different temporal morphologies (i.e., with…

astro-ph.HE2026

Constraining the Supernova Remnant Environment of FRB 190520B with Dispersion Measure and Scattering Timescale

Jia-Peng Wei, Chen Deng, Gwenael Giacinti +4

FRB 190520B is a repeating fast radio burst source whose large dispersion measure (DM) and temporal broadening suggest a dense and evolving local environment. In this work, we test…

astro-ph.HE2026

Gamma-Ray Bursts: Evidence for a Common Origin of X-ray Plateaus with Diverse Temporal Decay Index

Xiao-Fei Dong, Yong-Feng Huang, Chen Deng +8

A significant fraction of gamma-ray bursts (GRBs) exhibit a plateau in the early X-ray afterglow light curve, whose mechanism remains uncertain. While the post-plateau normal decay…

astro-ph.HE2026

Statistical analysis of multi-band plateaus in gamma-ray burst afterglows

Xiao-Yan Li, Tong Liu, Bao-Quan Huang +1

Plateau features are frequently observed in the afterglows of gamma-ray bursts (GRBs), yet their physical origins remain under debate. In this work, we compile a sample of 124 GRBs…