TITLE: GCN CIRCULAR NUMBER: 45293 SUBJECT: GRB 260730B: Glowbug gamma-ray detection DATE: 26/08/05 22:36:31 GMT FROM: C.C. Cheung at Naval Research Lab <Teddy.Cheung@nrl.navy.mil> 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 260730B, which was also detected by NuSTAR (GCN 45262), AstroSat (GCN 45265), and CALET (GCN 45284).  Using an adaptive window with a resolution of 32-ms, the burst onset is determined to be 2026-07-30 13:13:49.456 with a duration of 8.2 s and a total significance of about 21.8 sigma. The light curve comprises a multi-peaked structure corresponding to the brightest portion of the burst seen in the CALET light curve (GCN 45284).   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 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. View this GCN Circular online at https://gcn.nasa.gov/circulars/45293. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...