TITLE: GCN CIRCULAR NUMBER: 42143 SUBJECT: GRB 251005B: Glowbug gamma-ray detection DATE: 25/10/07 15:50:03 GMT FROM: C.C. Cheung at Naval Research Lab C.C. Cheung, R. Woolf, M. Kerr, J.E. Grove (NRL), A. Goldstein (USRA), C.A. Wilson-Hodge, D. Kocevski (MSFC), and M.S. Briggs (UAH) report: The Glowbug gamma-ray telescope [1,2,3], operating on the International Space Station, reports the detection of GRB 251005B, which was also detected by Fermi/GBM (GCN 42112). Using an adaptive window with a resolution of 32-ms, the burst onset is determined to be 2025-10-05 14:27:57.168 with a duration of 6.1 s and a total significance of about 14.1 sigma. The Glowbug onset is ~38 s after the Fermi/GBM trigger time (14:27:19) and corresponds to the second, brighter peak seen in the Fermi/GBM light curve. A search of the Glowbug data for the initial fainter peak at the Fermi/GBM T0 was inconclusive. The analysis results presented here are preliminary and use a response function that lacks a detailed characterization of the surrounding passive structure of the ISS. Glowbug is a NASA-funded technology demonstrator for sensitive, low-cost gamma-ray transient telescopes developed, built, and operated by the U.S. Naval Research Laboratory (NRL) with support from the University of Alabama in Huntsville, USRA, and NASA MSFC. It was launched on 2023 March 15 aboard the Department of Defense Space Test Program’s STP-H9 to the ISS, and operated until 2024 April when it was put in safe storage on orbit. Glowbug was recently removed from storage and resumed operation on 2025 September 12. [1] Grove, J.E. et al. 2020, Proc. Yamada Conf. LXXI, arXiv:2009.11959 [2] Woolf, R.S. et al. 2022, Proc. SPIE, 12181, id. 121811O [3] Woolf, R.S. et al. 2024, Proc. SPIE, 13151, id. 1315108 Distribution Statement A: Approved for public release. Distribution is unlimited.