Table 3
SDSS photometry of SN 2006oz (AB magnitudes).
| MJD | u | g | r | i | z |
|
|
|||||
| 54010.19 | >21.752 | >24.124 | >22.759 | >22.539 | >21.128 |
| 54012.18 | >21.803 | >21.650 | >22.360 | >21.805 | >21.321 |
| 54020.18 | >22.740 | >24.200 | >22.673 | >22.688 | >20.332 |
| 54022.23 | >22.228 | >23.674 | >22.898 | >22.772 | >20.815 |
| 54028.17 | 21.391 (0.198) | 22.280 (0.112) | 22.314 (0.237) | 22.359 (0.388) | >20.666 |
| 22.092 (0.856) | |||||
| 54030.18 | 21.823 (0.183) | 21.940 (0.067) | 21.926 (0.116) | 22.268 (0.230) | >21.293 |
| 22.683 (0.689) | |||||
| 54032.17 | ··· | 21.830 (0.217) | ··· | ··· | ··· |
| 54035.25 | >20.899 | 22.591 (0.266) | 22.451 (0.434) | 22.251 (0.425) | >20.184 |
| 21.763 (0.440) | 21.152 (0.514) | ||||
| 54037.16 | >21.795 | 22.240 (0.141) | 22.238 (0.320) | 21.858 (0.227) | >21.258 |
| 22.861 (0.595) | 23.096 (0.833) | ||||
| 54040.17 | >21.050 | 21.552 (0.216) | 21.567 (0.232) | 22.299 (0.515) | >20.602 |
| 22.490 (0.990) | 22.071 (0.904) | ||||
| 54047.16 | >20.364 | 20.924 (0.219) | 20.596 (0.174) | 20.872 (0.304) | >19.567 |
| 21.547 (0.713) | 21.306 (1.372) | ||||
| 54050.16 | 20.723 (0.114) | 20.534 (0.032) | 20.590 (0.051) | 20.666 (0.089) | 20.749 (0.378) |
| 54053.16 | 20.337 (0.082) | 20.283 (0.025) | 20.412 (0.040) | 20.507 (0.065) | 20.843 (0.318) |
| 54056.16 | 20.408 (0.172) | 20.160 (0.034) | 20.302 (0.059) | 20.694 (0.145) | 20.571 (0.368) |
| 54057.13 | 20.332 (0.067) | 20.089 (0.021) | 20.150 (0.033) | 20.370 (0.056) | 20.642 (0.225) |
| 54059.16 | 20.097 (0.079) | 20.011 (0.021) | 20.067 (0.035) | 20.177 (0.050) | 20.520 (0.225) |
| 54061.17 | 20.115 (0.079) | 19.964 (0.026) | 19.930 (0.034) | 20.122 (0.052) | 20.098 (0.184) |
| 54062.16 | 20.318 (0.092) | 19.927 (0.030) | 20.017 (0.038) | 20.226 (0.062) | 20.467 (0.285) |
| 54068.15 | ··· | 19.800 (0.079) | 19.810 (0.076) | 20.217 (0.161) | 19.909 (0.242) |
|
|
|||||
| 54367.02a | ··· | >24.508 | >24.209 | ··· | ··· |
| 54395.57b | >23.228 | ··· | ··· | >23.592 | >22.190 |
Notes. The quoted limits are 3σ. For the epochs after the SN discovery, where the SN was below the formal detection limit (u and z-band), we also provide, below the 3σ limits, the asinh magnitudes (Lupton et al. 1999; Holtzman et al. 2008), which were used as the best approximation in the construction of the bolometric light curve.
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