GCN Circular 45750
GRB 260924A: Extreme Isotropic-equivalent Gamma-ray Energy and encouragement for multiwavelength follow-up observations
From: Rahul Gupta at NASA GSFC
Issued: 2026-09-25 19:48 UTC
Type: GRB
Rahul Gupta (NASA GSFC), Peter Veres (UAH), Vikas Chand (LSU), Eric Burns (LSU), Pádraig McDermott (University College Dublin), and L. Scotton (UAH) reports:
We have estimated the isotropic-equivalent gamma-ray energy of GRB 260924A (The Fermi GBM team, GCN 45712; D'Elia et al., GCN 45713; Salunke et al., GCN 45720; Holzmann Airasca et al., GCN 45721; McDermott et al., GCN 45723; Waratkar et al., GCN 45732; Gupta et al., GCN 45733; and Yu et al., GCN 45741) using the time-integrated Fermi-GBM spectrum and the measured redshift of z = 3.51 (Castro-Tirado et al. GCN 45740). The time-averaged spectrum from T0-11.6 to T0+382.6 s is best fit by a Band function with Epeak = 645 +/- 4 keV, alpha = -0.91 +/- 0.01, and beta = -2.36 +/- 0.01 (McDermott et al., GCN 45723). Using the spectral parameters from McDermott et al., GCN 45723 and measured fluence of 2.84 × 10^-4 erg cm^-2 in the 10-1000 keV observer-frame energy range, and applying a bolometric k-correction to the 1-10,000 keV rest-frame energy range, we obtain an isotropic-equivalent gamma-ray energy of approximately 9.74 × 10^54 erg.
We adopted a flat Lambda-CDM cosmology with Omega_m = 0.286, Omega_Lambda = 0.714, and H0 = 69.6 km s^-1 Mpc^-1.
The inferred isotropic-equivalent energy places GRB 260924A among the most energetic gamma-ray bursts known. Its energetics are comparable, within the uncertainties, to those of GRB 221009A, the “BOAT” (Brightest Of All Time).
Given its extreme energetics and broad observational coverage, continued multi-wavelength observations of GRB 260924A are strongly encouraged.
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.
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Transient Alerts » in reply to GRB 260924A
GRB 260924A: Extreme Isotropic-equivalent Gamma-ray Energy and encouragement for multiwavelength follow-up observations
The whole thread (28 posts)
- GRB 260924A
- GRB 260924A: VLA detection
- GRB 260924A: Swift/UVOT UV grism spectrum results
- GRB 260924A: AbAO optical observations
- GRB 260924A: Upper limits from a neutrino search with IceCube
- GRB 260924A: Near-infrared detection with MDM/MIRAGE
- GRB 260924A: COLIBRÍ optical observations
- GRB 260924A: Second-epoch J-band upper limit from the SYSU 80 cm infrared telescope
- Konus-Wind detection of GRB 260924A
- GRB 260924A: Extreme Isotropic-equivalent Gamma-ray Energy and encouragement for multiwavelength follow-up observations
- GRB 260924A: Optical follow-up observations with Kinder
- GRB 260924A: Ondrejov D50 optical afterglow detection
- GRB 260924A: SVOM/GRM observation
- GRB 260924A: 2.2m CAHA spectroscopic redshift z = 3.51
- GRB 260924A: J-band observations by the SYSU 80 cm infrared telescope
- GRB 260924A: Swift/UVOT Detection
- GRB 260924A: GROWTH-India Telescope optical observations
- GRB 260924A: Swift-BAT refined analysis
- GRB 260924A: NuSTAR detection of prompt emission
- GRB 260924A: Swift/UVOT Upper Limits
- GRB 260924A: Swift-XRT refined Analysis
- GRB 260924A: Fermi GRB Observation
- GRB 260924A: Fermi-LAT detection of a bright burst
- GRB 260924A: AstroSat CZTI detection
- GRB 260924A: NOT optical counterpart confirmation
- GRB 260924A: detection of a bright optical afterglow by the 1.5m OSN telescope
- GRB 260924A: Enhanced Swift-XRT position
- GRB 260924A: Swift detection of a burst
