GCN Circular 38621
Subject
GRB 241217A / EP241217b: NOT optical upper limits
Event
Date
2024-12-18T14:57:47Z (a year ago)
Edited On
2025-10-23T22:15:48Z (2 months ago)
From
Zipei Zhu at NAOC <zpzhu@nao.cas.cn>
Edited By
Vidushi Sharma at NASA GSFC/UMBC <vidushi.sharma@nasa.gov> on behalf of Daniele Bjørn Malesani at Cosmic Dawn Center, Niels Bohr Institute <daniele.malesani@nbi.ku.dk>
Via
legacy email
Z.P. Zhu, X. Liu, D. Xu (NAOC), D. B. Malesani (DAWN/NBI and Radboud Univ.), A. Amanda Djupvik (NOT), Laura Cotter, Antonio Martin-Carrillo (UCD), Jesse Palmerio (CEA/Irfu) and Susanna D. Vergani (GEPI / Obs. de Paris) report on behalf of a large collaboration:
We observed the field of GRB 241217A / EP241217b detected by SVOM (Brunet et al., GCN 38594) and Einstein Probe (Zhou et al., GCN 37492), using the StanCam and NOTCam instruments mounted on the Nordic Optical Telescope (NOT), with 9x200s in the SDSS-z band and 18x60 s photometry in the J band. Observations started at 23:09:34 UT on 2024-12-17, i.e. 6.2 hr after the trigger.
The optical afterglow (Qiu et al., GCN 38600) is not detected in any of the stacked images, down to the following 5-sigma upper limits:
T_mid (UT) | T_mid (hr) | filter | Exposue|5-sigma U.L. (AB)
2024-12-17T23:20:59 | 6.396 | J | 18x60s | 19.5
2024-12-18T01:05:01 | 8.130 | z | 9x200s | 21.3
calibrated with nearby Pan-STARRS and 2MASS stars, and not accounting for any Galactic extinction correction.