Deciphering the Physical Origin of GRB 240825A: A Long GRB Lacking a Bright Supernova
astro-ph.HE
Submitted: 2025-07-31
Updated: 2026-09-22
Comments: 30 pages, 21 figures, 6 tables, accepted for publication in ApJ
Project page: https://iraf-community.github.io
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Fermi-GBM Observations of GRB 230307A: An Exceptionally Bright Long-Duration Gamma-ray Burst with an Associated Kilonova
- Multiwavelength Observations of Gamma Ray Bursts
- An Intermediate Luminosity GRB 210210A: The early onset of the external forward shock in the X-ray?
- Time-resolved spectro-polarimetric analysis of extremely bright GRB 230307A: Possible Evidence of evolution from photospheric to synchrotron dominated emission
- The ASIM Mission on the International Space Station
- GRB 240825A: Early Reverse Shock and Its Physical Implications
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