Table A.2
GROND photometry of XRF 100316D/SN 2010bh after image subtraction.
| Time Interval | g′ | r′ | i′ | z′ | J | H |
| [d] after the trigger | ||||||
|
|
||||||
| 0.49023–0.49470 | 20.75(04) | 20.90(04) | 20.87(05) | 20.77(07) | 20.69(14) | > 20.04 |
| 0.56046–0.60240 | 20.81(03) | 20.91(03) | 20.94(04) | 20.76(04) | 20.71(26) | > 20.67 |
| 1.47634–1.49123 | 20.75(04) | 20.90(04) | 20.59(05) | 20.51(05) | 20.47(22) | 20.69(33) |
| 1.69356–1.70396 | 20.92(04) | 20.77(03) | 20.69(05) | 20.65(06) | 20.40(32) | > 20.09 |
| 2.49804–2.51041 | 20.70(04) | 20.58(04) | 20.50(05) | 20.20(04) | 19.99(17) | > 20.09 |
| 3.50557–3.52164 | 20.67(03) | 20.40(03) | 20.24(03) | 19.94(03) | 19.72(17) | 19.94(21) |
| 4.48027–4.48963 | 20.43(04) | 20.21(03) | 20.15(04) | 19.78(04) | 20.00(19) | 20.22(23) |
| 5.46324–5.47229 | 20.33(04) | 20.11(04) | 20.04(04) | 19.61(04) | 19.93(19) | 19.92(23) |
| 7.47679–7.48174 | 20.26(06) | 19.96(04) | 19.87(06) | 19.58(06) | 19.69(19) | 20.20(28) |
| 10.47338–10.48259 | 20.38(03) | 19.91(03) | 19.98(04) | 19.37(03) | 19.53(14) | 19.85(25) |
| 11.47550–11.47994 | 20.50(03) | 20.01(03) | 19.99(04) | 19.33(03) | 19.49(14) | 19.94(18) |
| 14.47912–14.49638 | 20.71(04) | 20.07(03) | 20.08(03) | 19.38(03) | 19.51(12) | 19.67(22) |
| 15.48101–15.48997 | 20.72(05) | 20.07(04) | 20.16(05) | 19.32(04) | 19.59(13) | 19.85(19) |
| 19.52885–19.53123 | 21.33(10) | 20.36(05) | 20.39(07) | 19.51(05) | 19.70(19) | > 19.71 |
| 21.48630–21.49543 | 21.52(06) | 20.48(04) | 20.48(04) | 19.65(03) | 19.64(13) | 19.95(19) |
| 25.49771–25.51874 | 21.91(05) | 20.78(03) | 20.66(03) | 19.87(03) | 19.67(13) | 20.30(21) |
| 32.48587–32.50697 | 22.78(10) | 21.42(04) | 21.28(05) | 20.39(04) | 20.07(19) | > 20.41 |
| 40.46892–40.50042 | > 23.11 | 21.83(06) | 21.74(07) | 20.81(05) | > 20.34 | > 20.43 |
| 83.43058–83.45161 | > 23.95 | 23.66(23) | > 22.91 | 22.78(25) | > 20.95 | > 20.90 |
Notes. The template image for subtraction was taken 234 days after burst. The time reference is t0 = 55 271.53113 MJD, the date of the GRB trigger. All magnitudes are in the AB system and corrected for neither Galactic nor host-galaxy extinction. Upper limits are all at the 3σ confidence level. Errors include the systematics of the photometric calibration.
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