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Table B.1.

Observed GROND magnitudes of the GRB 100418A afterglow for the seven highlighted epochs in light blue and light red in Fig. 2.

SED mid-time [ks] g′(mAB) r′(mAB) i′(mAB) z′(mAB) J(mVega) H(mVega) Ks(mVega)
I* 27.7 18.99±0.05 18.64±0.05 18.33±0.07 18.08±0.07 17.63±0.07 17.26±0.08 17.18±0.14
II* 40.2 19.11±0.05 18.48±0.07 18.77±0.06 18.24±0.07 17.81±0.09 17.49±0.10 17.15± 0.12

I 130.9 20.20±0.06 19.87±0.06 19.56±0.07 19.36±0.07 18.93±0.09 18.66±0.12 18.34±0.11
II 202.1 20.92±0.06 20.60±0.06 20.27±0.06 20.01±0.07 19.66±0.09 19.51±0.11 19.12±0.16
III 217.8 21.07±0.07 20.73±0.07 20.36±0.06 20.22±0.08 19.85±0.10 19.55±0.13 19.22±0.18
IV 296.8 21.34±0.06 21.13±0.07 20.72±0.07 20.59±0.07 20.07±0.11 19.91±0.16 19.72±0.14
V 476.4 21.96±0.05 21.60±0.04 21.36±0.06 21.09±0.08 20.53±0.17 20.18±0.16 19.98 UL

host 22.82±0.06 22.36±0.06 22.25±0.07 22.14±0.07 21.95±0.08 21.70±0.18 21.68±0.25

Notes. Two epochs during the energy injection phase and five epochs after the break in the light curve. The host contribution was subtracted for each band. The Galactic foreground extinction is A v Gal = 0.22 $ A^{\mathrm{Gal}}_{\mathrm{v}}=0.22 $ mag.

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