{
  "format": "text/plain",
  "body": "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:\n\nThe Glowbug gamma-ray telescope [1,2,3], operating on the International Space Station, confirms the detection of the short GRB 251129B, which was detected by AstroSat/CZTI (GCN 42958), Konus-Wind, Swift/BAT, Mars-Odyssey/HEND (GCN 42960), and GECAM-B (GCN 42984). The light curve comprises a single peak at 2025-11-29 09:51:33.20 with a duration of 0.16s.\n\nThe analysis results presented here are preliminary and use a response function that lacks a detailed characterization of the surrounding passive structure of the ISS.\n\nGlowbug 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.\n\n[1] Grove, J.E. et al. 2020, Proc. Yamada Conf. LXXI, arXiv:2009.11959\n[2] Woolf, R.S. et al. 2022, Proc. SPIE, 12181, id. 121811O\n[3] Woolf, R.S. et al. 2024, Proc. SPIE, 13151, id. 1315108\n\nDistribution Statement A: Approved for public release.  Distribution is unlimited.",
  "bibcode": "2025GCN.42992....1C",
  "eventId": "GRB 251129B",
  "createdOn": 1764882234833,
  "submitter": "C.C. Cheung at Naval Research Lab <Teddy.Cheung@nrl.navy.mil>",
  "subject": "GRB 251129B: Glowbug gamma-ray detection of a short burst",
  "submittedHow": "web",
  "circularId": 42992
}