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Table A.3.

GROND photometry and the X-ray time interval used for the SED fitting of the final 10 GRBs.

GRB g r i z J H Ks X-ray time interval Δt c (h)
0901021 20.98±0.03b 20.64±0.03b 20.03±0.03b 19.64±0.03b 19.03±0.04b 18.25±0.07b 17.59±0.07b 1.48-7.26
0806052 20.76±0.05 20.15±0.05 19.66±0.05 19.35±0.05 19.01±0.09 18.56±0.09 18.26±0.11 1.67-5.56
120119A4 d 18.8±0.1 17.7±0.1 16.8±0.1 16.2±0.1 15.2±0.1 14.6±0.1 14.0±0.1 0.39-2.5
121027A5 d 22.1±0.2 21.6±0.1 21.3±0.1 20.9±0.1 20.4±0.1 19.7±0.1 19.7±0.1 62.5-152.78
150206A6 d 22.6 0.2 21.9 0.1 21.2 0.1 20.8 0.1 20.0 0.2 > 20.2 > 19.4 9.27-11.33
180325A7 20.44±0.04 19.56±0.03 19.16±0.03 18.29±0.03 17.42±0.05 16.84±0.05 16.38±0.07 1.32-1.93
0708028 23.16±0.42a 21.46±0.16a 21.66±0.1a 20.41±0.15a 19.52±0.1a 18.92±0.12a 18.29±0.13a 1.11-119.44
0908129 d 22.15±0.15 21.50±0.08 21.30±0.13 21.02±0.12 20.57±0.15 > 19.8 > 18.9 2.78-69.44
151112A10 > 25.4 23.58±0.09 22.63±0.08 22.23±0.09 21.74±0.26 21.25±0.22 20.59±0.26 5.67-10.75
100219A10 > 24.2 22.77±0.09 21.37±0.06 21.24±0.08 20.72±0.20 20.23±0.19 20.12±0.34 2.78-8.33

Notes: Magnitudes are in the AB system unless otherwise indicated. aMagnitudes already corrected for the Galactic foreground reddening. b Vega magnitude system. cTime interval at which the X-ray spectrum has been created and used for the broad-band SED. dData from GCN circulars.

1Gendre et al. (2010); 2Zafar et al. (2012); 4Schady et al. (2012b); 5Sudilovsky et al. (2012); 6Schweyer et al. (2015); 8Krühler et al. (2008); 9Updike et al. (2009); 10Bolmer et al. (2018)

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