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Table C.1

Light curve models and parameters used to flux normalize XRT X-ray and GROND NIR/optical data to a common reference time.

Model α 1 α 2 α 3 t break Host Additional dataa
(ks) (y/n) (reference)
GRB 071025
NIR/opt. PL 1.32 ± 0.11 ... ... ... no PAIRTEL JHKs (1)
X-ray PL 1.60 ± 0.01 ... ... ...
GRB 080825Bb
NIR/opt. BRPL 1.1 ± 0.1 2.2 ± 0.6 ... 59 ± 24 no DFOSC I(2)
X-ray PL 1.8 ± 0.6 ... ... ...
GRB 080913
NIR/opt. PL 1.13 ± 0.08 ... ... ... no
X-ray PL 1.22 ± 0.06 ... ... ...
GRB 080916C
NIR/opt. PL 1.73 ± 0.39 ... ... ... no
X-ray PL 1.30 ± 0.09 ... ... ...
GRB 090205
NIR/opt. PL 1.35 ± 0.04 ... ... ... yes FORS1 RI (3)
X-ray BRPL 0.91 ± 0.03 2.12 ± 0.07 ... 23 ± 1
GRB 090423
NIR/opt. BRPL 0.05 ± 0.01 1.00 ± 0.03 ... 24 ± 8 no HAWKI KJ/WFCAM K
X-ray PL + BRPL 1.38 ± 0.04 −3.75 ± 4.20 1.34 ± 0.15 3.0 ± 4.6 NIRI HJ/ISAAK J (4)(5)
GRB 090429Bc
NIR/opt. PL 0.61 ± 0.08 ... ... ... no NIRI JHK (6)
X-ray BRPL −1.14 ± 0.59 1.37 ± 0.10 ... 0.65 ± 0.18
GRB 090516A
NIR/opt. PL 1.72 ± 0.05 ... ... ... yes FORS2 R (7)/NOT R (8)
X-ray BRPL 0.78 ± 0.06 1.75 ± 0.05 ... 16 ± 1
GRB 100219A
NIR/opt. PL 1.68 ± 0.46 ... ... ... yes HAWKI KHJ/GMG r′
X-ray BRPL 1.72 ± 0.25 > 3.0 ... ... GTC i′ (9)
GRB 100513A
NIR/opt. PL 0.48 ± 0.17 ... ... ... no PAIRITEL JHKs (10)
X-ray PL 0.96 ± 0.06 ... ... ...
GRB 100905A
NIR/opt. PL 0.60 ± 0.06 ... ... ... no
X-ray PL 0.88 ± 0.03 ... ... ...
GRB 111008A
NIR/opt. PL 1.02 ± 0.06 ... ... ... no
X-ray BRPL 0.97 ± 0.09 1.42 ± 0.05 ... 41 ± 11
GRB 120712A
NIR/opt. BRPL 0.04 ± 0.08 1.66 ± 0.16 ... 102 ± 13 no
X-ray BRPL 0.95 ± 0.03 1.80 ± 0.11 ... 6 ± 1
GRB 130606A
NIR/opt. PL 1.71 ± 0.03 ... ... ... no NOT r′i′z′/TNG i′z′ (11)
X-ray PL 1.71 ± 0.03 ... ... ... GTC i′z′ (12)
GRB 131117A
NIR/opt. PL 0.86 ± 0.01 ... ... ... no
X-ray PL + G 0.95 ± 0.02 ... ... ...
GRB 140304A
NIR/opt. PL + BRPL 2.25 ± 0.24 −7.42 ± 5.94 1.86 ± 0.20 25 ± 2 no RATIR grizJH (13)
X-ray PL + BRPL 1.93 ± 0.14 −9.71 ± 6.89 1.50 ± 0.09 16 ± 2 Nanshan R (14)/NOT gr (15)
MONDY R(16)/ORI-40 R (17)
GRB 140311A
NIR/opt. PL 0.95 ± 0.04 ... ... ... no NOT r′i′ (18)
X-ray BRPL 1.20 ± 0.07 1.97 ± 0.58 ... 121 ± 65
GRB 140428A
NIR/opt. PL 1.81 ± 0.08 ... ... ... no OSN I (19)
X-ray BRPL 0.96 ± 0.07 > 2.0 ... 19 ± 9 LRIS i (20)
GRB 140515A
NIR/opt. BRPL 0.77 ± 0.25 > 2.5 ... ... no GMOS z′ (21)
X-ray PL + BRPL 3.10 ± 0.19 −3.77 ± 0.69 1.03 ± 0.05 2.3 ± 0.2 Chandra (22)
GRB 140614A
NIR/opt. PL 1.20 ± 0.04 ... ... ... no
X-ray PL + BRPL 1.92 ± 0.07 −0.27 ± 0.32 1.49 ± 0.08 7 ± 1
GRB 151027B
NIR/opt. BRPL 0.44 ± 0.19 1.44 ± 0.14 ... 34 ± 28 no NOT R (23)
X-ray BRPL 0.44 ± 0.19 1.44 ± 0.14 ... 34 ± 28 RATIR r′i′ (24)
GRB 151112A
NIR/opt. BRPL 0.84 ± 0.06 2.10 ± 0.29 ... 128 ± 14 no
X-ray BRPL 0.84 ± 0.06 > 1.2 ... 128 ± 14

Notes.

(a)

GROND optical and near-infrared data were extended with data collected from GCNs and refereed publications. The magnitudes were, if necessary, converted to the AB system.

(b)

The XRT light curve is also consistent with the model for the NIR/optical afterglow (see Fig. B.2).

(c)

We used the temporal decay slope as derived from the NIRI K band data to re-scale the NIRI J, H, and K-band observation to a common reference time (see Fig. B.7).

Reference. (1) Perley et al. (2010); (2) Thoene et al. (2008); (3) D’Avanzo et al. (2010); (4) Tanvir et al. (2009); (5) Salvaterra et al. (2009); (6) Cucchiara et al. (2011); (7) Gorosabel et al. (2009); (8) de Ugarte Postigo et al. (2009); (9) Thöne et al. (2013); (10) Morgan et al. (2010); (11)Hartoog et al. (2015); (12) Castro-Tirado et al. (2013); (13) Butler et al. (2014); (14) Xu et al. (2014b); (15) de Ugarte Postigo et al. (2014); (16) Volnova et al. (2014a); (17) Volnova et al. (2014b); (18) Xu et al. (2014a); (19) Aceituno et al. (2014); (20) Perley (2014a); (21) Melandri et al. (2015); (22) Margutti et al. (2014); (23) Malesani et al. (2015b); (24) Watson et al. (2015a).

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