Abstract
We report on the detection of candidate optical counterpart GOTO23akf/AT2023shv to the GRB 230911A with the Gravitational-wave Optical Transient Observer (GOTO) instruments located at La Palma, Canary Islands, and Siding Spring Observatory, Australia. The Fermi Gamma-ray Burst Monitor, which finds gamma-ray bursts (GRBs) nearly every two days, detected GRB 230911A with a statistical uncertainty of 4.°1. However, the large (∼10–100 deg2) localization areas mostly impede the rapid identification of an optical counterpart. GOTO facilities fully covered 90% localization area of the GRB 230911A. We proposed GOTO23akf as the optical afterglow of GRB 230911A, subsequently confirmed through Swift-X-Ray Telescope observations in which an uncatalogued X-ray source spatially coincident with the GOTO candidate was detected. This is the first optical afterglow discovery for a Fermi GRB with the newly expanded GOTO network.
Original language | English |
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Article number | 6 |
Pages (from-to) | 1-4 |
Number of pages | 4 |
Journal | Research Notes of the American Astronomical Society |
Volume | 8 |
Issue number | 1 |
Early online date | 4 Jan 2024 |
DOIs | |
Publication status | Published - 4 Jan 2024 |
Keywords
- Optical observation
- Gamma-ray bursts