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Table A.2.
Optical photometry of the local sequence for SN 2014ab in the “standard” system.
| ID | α (2000) | δ (2000) | B | V | u′ | g′ | r′ | i′ |
|---|---|---|---|---|---|---|---|---|
| 1 | 207.103256 | 7.430505 | 14.464(011) | 13.444(023) | 16.446(044) | 13.917(012) | 13.080(018) | 12.797(009) |
| 2 | 207.016541 | 7.351987 | 14.614(015) | 13.689(015) | 16.259(038) | 14.130(016) | 13.290(016) | 12.963(009) |
| 3 | 207.015869 | 7.294901 | 14.590(016) | 13.720(012) | 16.146(012) | 14.119(011) | 13.414(008) | 13.161(006) |
| 4 | 207.114792 | 7.291261 | 15.526(023) | 14.808(022) | 16.747(049) | 15.147(028) | 14.583(017) | 14.361(015) |
| 5 | 207.009033 | 7.314421 | 16.291(023) | 15.588(018) | 17.388(055) | 15.904(019) | 15.344(016) | 15.145(014) |
| 6 | 207.011932 | 7.279015 | 16.564(024) | 15.738(011) | 17.678(082) | 16.132(023) | 15.420(007) | 15.151(006) |
| 7 | 207.056549 | 7.408627 | 17.366(107) | 16.557(053) | 18.886(080) | 16.966(029) | 16.254(035) | 15.985(021) |
| 8 | 207.066711 | 7.456894 | 17.197(040) | 16.651(063) | 17.893(045) | 16.893(050) | 16.533(038) | 16.401(037) |
| 9 | 206.970734 | 7.467194 | 17.873(095) | 16.667(049) | 20.172(175) | 17.312(076) | 16.086(020) | 15.526(021) |
| 10 | 206.985626 | 7.469990 | 17.387(093) | 16.748(044) | 18.374(047) | 17.066(053) | 16.548(034) | 16.378(036) |
| 11 | 207.005112 | 7.462066 | 17.547(076) | 16.980(068) | 18.446(177) | 17.231(050) | 16.807(047) | 16.680(051) |
| 12 | 207.083344 | 7.439429 | 17.800(123) | 17.094(045) | 18.862(072) | 17.432(045) | 16.804(053) | 16.574(035) |
| 13 | 207.017670 | 7.366422 | 17.598(063) | 17.004(032) | 18.429(073) | 17.302(041) | 16.820(037) | 16.564(043) |
| 14 | 207.042816 | 7.346911 | 17.631(082) | 17.268(079) | 18.254(360) | 17.414(081) | 17.191(062) | 17.105(065) |
| 15 | 207.089340 | 7.359910 | 17.796(093) | 17.428(077) | 17.735(102) | 17.632(061) | 17.415(070) | 17.500(060) |
| 16 | 206.964035 | 7.465946 | 17.983(056) | 17.435(057) | 18.840(110) | 17.674(050) | 17.280(060) | 17.103(082) |
| 17 | 207.051956 | 7.360322 | 18.002(088) | 17.609(058) | 18.643(084) | 17.769(036) | 17.461(051) | 17.394(094) |
| 18 | 207.099777 | 7.315611 | 18.480(085) | 17.496(060) | ... | 18.019(075) | 17.077(052) | 16.648(038) |
| 19 | 207.090088 | 7.375126 | 18.332(037) | 17.644(083) | 19.249(020) | 17.987(091) | 17.401(066) | 17.143(065) |
| 20 | 206.999039 | 7.336068 | 18.927(048) | 17.627(049) | ... | 18.281(056) | 17.015(036) | 16.112(028) |
| 21 | 207.094254 | 7.321296 | 19.040(093) | 17.863(081) | ... | 18.449(077) | 17.279(072) | 16.671(040) |
| 22 | 207.026749 | 7.289460 | 19.266(047) | 17.956(091) | ... | 18.602(057) | 17.344(086) | 16.760(047) |
| 23 | 207.071671 | 7.423058 | 18.691(154) | 18.198(109) | 19.223(054) | 18.381(053) | 17.966(113) | 17.762(075) |
Notes. Values in parenthesis are 1-σ uncertainties that correspond to the rms of the instrumental errors of the photometry obtained over a minimum of three nights observed relative to standard star fields.
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