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Table B.2.

Observed magnitudes of the GRB 100418A afterglow during the epochs for the broadband analysis (as highlighted in Fig. 2).

SED mid-time [ks] g′(mAB) r′(mAB) i′(mAB) z′(mAB) J(mVega) H(mVega) Ks(mVega)
I 173 20.59±0.05 20.26±0.04 19.95±0.06 19.72±0.08 19.31±0.13 18.99±0.15 18.67±0.24
II 259 21.21±0.04 20.88±0.04 20.57±0.06 20.34±0.08 19.92±0.14 19.61±0.15 19.28±0.23
III 450 21.84±0.05 21.51±0.04 21.31±0.06 21.18±0.07 20.55±0.13 19.89±0.15 > 20.12
IV 1065 23.35±0.05 23.02±0.05 22.71±0.07 22.48±0.08 22.06±0.14 21.75±0.14 > 21.42
V 1555 23.92±0.05 23.59±0.05 23.28±0.06 23.05±0.09 22.63±0.14 22.33±0.15 > 21.99
VI 2246 24.48±0.06 24.15±0.04 23.84±0.07 23.61±0.08 23.18±0.16 22.88±0.18 > 22.56
VII 3283 25.05±0.05 24.72±0.06 24.42±0.07 24.18±0.09 23.76±0.16 23.46±0.17 > 23.13
VIII 5788 25.91±0.07 25.58±0.06 25.27±0.08 25.05±0.10 24.62±0.15 24.32±0.17 > 23.99

Notes. The host contribution was subtracted and the magnitudes were corrected for A v Gal $ A^{\mathrm{Gal}}_{\mathrm{v}} $=0.22 mag.

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