Fires in the deep: The luminosity distribution of early-time gamma-ray-burst afterglows in light of the Gamow Explorer sensitivity requirements

Open Access

Table B.1

GRB afterglow/supernova/host observations.

GRB	∆t (days)	mag	filter	Telescope/Instrument
080413A	0.061861	${19.249}_{- 0.212}^{+ 0.263}$ $19.249_{ - 0.212}^{ + 0.263}$	b	Swift UVOT
	1.587929	> 22.091	b UL	Swift UVOT
	1.718968	> 21.616	b UL	Swift UVOT
	0.003005	${14.605}_{- 0.091}^{+ 0.099}$ ${14.605_{ - 0.091}^{ + 0.099}}$	υ	Swift UVOT
	0.003177	${14.701}_{- 0.068}^{+ 0.072}$ ${14.701_{ - 0.068}^{ + 0.072}}$	υ	Swift UVOT

Notes. This table is available in its entirety at the CDS. All data are in AB magnitudes and not corrected for Galactic foreground extinction. Midtimes are derived logarithmically. $t = 10^{([\log (t_{1} - t_{0}) + \log (t_{2} - t_{0})] / 2)}$ $t = {10^{\left( {\left[ {\log \left( {{t_1} - {t_0}} \right) + \log \left( {{t_2} - {t_0}} \right)} \right]/2} \right)}}$ , hereby t_1,2 are the absolute start and stop times, and t₀ is the GRB trigger time.

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