Broad-band modelling of the GRB 230812B afterglow: Implications for very-high-energy γ-ray detections with IACTs

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Table B.1.

Isotropic-equivalent energy (E_γ) and fluence from various instruments of GRB 230812B reported in literature from various instruments.

Instrument	Energy band	Fluence (ℱ_γ)	E_γ	Reference
[× 10⁻⁴ erg cm⁻²]	[×10⁵²erg]
Fermi/GBM	10-1000 keV	2.52	8.3	Roberts et al. 2023,
Fermi/GBM	10-1000 keV	2.52	8.3	de Ugarte Postigo et al. 2023

Konus-Wind	20-10000 keV	3.27 ± 0.07	10.9 ± 0.2	Frederiks et al. 2023a,b

GRID	10-1000 keV	$1 . 41_{- 0.13}^{+ 0.08}$ $1.41_{-0.13}^{+0.08}$	$9 . 7_{- 0.5}^{+ 0.1}$ $9.7_{-0.5}^{+0.1}$	Table 1 of Wang et al. 2025

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