collaborators

5 papers

astro-ph.HE2026

Revealing the high redshift host galaxy of the short GRB 061201 with JWST

Yuhan Mao, Hanrui He, Jia Ren +6

Using deep near-infrared and optical images from JWST and HST, we identify a new host galaxy candidate for GRB 061201. It lies ~2" from the optical afterglow position. Photometric…

astro-ph.HE2026

Neutron Star Merger Rates from Multi-messenger Observations: Clues to the Physical Origin of the Short and Long-short Gamma-ray Bursts

Zhi-Ping Jin, Yuan-Zhu Wang, Yin-Jie Li +4

Short and long-short gamma-ray bursts (GRBs) are widely believed to be powered by neutron star mergers. In this work, we calculate local rate of such GRBs and find a relatively hig…

astro-ph.HE2026

An extreme particle accelerator powered by pulsar PSR J1849-0001

The LHAASO Collaboration

Pulsar wind nebulae (PWNe) are bubbles of relativistic particles, powered by the rotational energy loss of the central pulsars. The Crab Nebula, powered by the Milky Way's most ene…

astro-ph.HE2026

Illuminating the Mass Gap Through Deep Optical Constraint on a Neutron Star Merger Candidate S250206dm

Zhengyan Liu, Zelin Xu, Ji-an Jiang +35

The gravitational wave (GW) event S250206dm, as the first well-localized neutron star merger candidate potentially located in the mass gap, presented a unique opportunity to probe…

astro-ph.HE2025

Probable evidence for a transient mega-electron volt emission line in the GRB 221023A

Lu-Yao Jiang, Yun Wang, Yu-Jia Wei +6

Detection of spectral line in gamma-ray bursts (GRBs) is importance for studying GRB physics, as it provides insights into the composition and physical conditions of the GRB enviro…