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Table A.2

UVOT observations of the GRB 130603B afterglow.

Mid t − t0 Half bin width AB mag Mag error Filter
(s) (s)

137 75 21.56 +0.35, –0.26 white
651 97 >20.47 white
5599 818 21.60 +0.21, –0.18 white
51 526 170 21.99 +0.34, –0.26 white
696 91 >18.15 V
7745 2552 >19.57 V
37 325 9331 >20.18 V
627 96 >19.84 B
8450 3874 20.81 +0.26, –0.21 B
42 451 8900 >20.82 B
487 212 >20.68 U
5189 818 >20.80 U
80 635 40 241 >21.63 U
134 782 9495 >22.31 U
664 10 >19.60 UVW1
4984 818 >21.42 UVW1
29 117 11 270 >22.35 UVW1
112 413 32582 23.05 +0.28, –0.22 UVW1
640 10 >20.54 UVM2
4778 819 >21.40 UVM2
27 494 11 986 22.54 +0.32, –0.25 UVM2
677 97 >20.68 UVW2
5772 783 >21.8 UVW2
36 426 9338 >22.66 UVW2
270 445 17351 >23.12 UVW2

Notes. Column 1: mid-time of exposure, in seconds, since BAT trigger; Col. 2: half bin width; Col. 3: AB magnitude; Col. 4: magnitude error; Col. 5: UVOT filter. When the signal to noise is below 3, a 3σ upper limit is given.

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