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GRB 260924A: detection of a bright optical afterglow by the 1.5m OSN telescope

GCN Circular 45717
GRB 260924A: detection of a bright optical afterglow by the 1.5m OSN telescope
From: Alberto Castro-Tirado at Inst.de Astro. de Andalucia
Issued: 2026-09-24 07:10 UTC

Y.-D. Hu (GXI), A. Sota, E. Fernandez-Garcia, A. J. Castro-Tirado, I. Perez-Garcia, M.D. Caballero-Garcia and M. Gritsevich (IAA-CSIC), on behalf of a larger collaboration, report:

Following the detection of GRB 260924A by both Fermi (Fermi team, GCN 45712) and Swift (D'Elia et al. GCN 45713), we triggered the 1.5m telescope at Sierra Nevada Observatory (OSN) in Granada (Spain), starting on Sep 24, 04:24 UT (~3.18 h post trigger) in the BVRI filters. An uncatalogued object is detected within the XRT error circle (Evans et al. GCNC 45715) with R=15.5+-0.1 mag (calibrated with USNO B2), which we propose to be the GRB 260924A optical afterglow. Spectroscopic observations are encouraged.

We thank the staff at OSN for their excellent support.

Filter: gamma-ray bursts are posted only if in the top 10% of the past year's — by fluence (total energy received per cm², from Fermi GBM, Konus-Wind, GECAM and similar circulars; now ≥ 3.9×10^-5 erg/cm²) or by the number of GCN Circulars about the burst (now ≥ 14). Thresholds are recalculated monthly.
Relayed automatically from NASA's General Coordinates Network.

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