Table C.1.
Optical (BVuriz) photometric measurements of AT 2010dn.
Date | MJD | Phasea | B(err) | V(err) | u(err) | r(err)bc | i(err)b | z(err) | Instrument |
---|---|---|---|---|---|---|---|---|---|
20010302 | 51970.50 | -3384.4 | – | > 24.1 | – | – | – | – | 1 |
20090330 | 54921.11 | -433.8 | – | – | – | > 19.0 | – | – | 2 |
20100521 | 55338.00 | -16.9 | – | – | – | > 18.0 | – | – | 2 |
20100531 | 55348.04 | -6.9 | – | – | – | 17.546(0.123) | – | – | 2 |
20100601 | 55348.98 | -5.9 | – | – | – | 17.407(0.211) | – | – | 2 |
20100601 | 55349.45 | -5.4 | – | – | – | 17.593(0.172) | – | – | ALFOSC |
20100602 | 55350.36 | -4.5 | – | – | – | 17.41 | – | – | 3 |
20100603 | 55350.65 | -4.2 | – | 17.4 | – | – | – | – | 4 |
20100603 | 55350.99 | -3.9 | – | – | – | 17.412(0.266) | – | – | 2 |
20100603 | 55351.40 | -3.5 | 18.036(0.028) | 17.649(0.051) | 18.780(0.105) | 17.465(0.040) | 17.379(0.043) | – | LRS |
20100605 | 55352.85 | -2.0 | 17.923(0.036) | 17.411(0.044) | 18.700(0.206) | 17.346(0.040) | 17.260(0.036) | 17.252(0.065) | EM01 |
20100607 | 55355.42 | +0.5 | 17.781(0.046) | 17.298(0.047) | 18.677(0.080) | 17.215(0.060) | 17.292(0.040) | – | LRS |
20100609 | 55357.40 | +2.5 | – | – | – | 17.264(0.167) | – | – | ALFOSC |
20100611 | 55359.40 | +4.5 | 18.102(0.034) | 17.584(0.017) | – | 17.477(0.037) | 17.370(0.017) | – | RATCam |
20100611 | 55359.43 | +4.5 | 18.066(0.047) | 17.481(0.092) | – | 17.424(0.086) | 17.347(0.052) | – | LRS |
20100612 | 55360.41 | +5.5 | 18.074(0.016) | 17.607(0.029) | – | 17.498(0.018) | 17.386(0.038) | – | RATCam |
20100613 | 55361.45 | +6.6 | 18.177(0.021) | 17.638(0.025) | 18.990(0.207) | 17.490(0.032) | 17.430(0.039) | 17.486(0.073) | RATCam |
20100616 | 55363.84 | +8.9 | 18.141(0.053) | 17.663(0.031) | 19.158(0.358) | 17.552(0.034) | 17.467(0.038) | 17.366(0.048) | EM01 |
20100616 | 55364.39 | +9.5 | – | – | – | 17.669(0.248) | – | – | LRS |
20100617 | 55365.40 | +10.5 | 18.139(0.028) | 17.730(0.025) | 19.237(0.114) | 17.605(0.057) | 17.495(0.040) | 17.376(0.060) | RATCam |
20100618 | 55366.38 | +11.5 | 18.294(0.029) | 17.790(0.028) | – | 17.607(0.031) | 17.486(0.039) | – | RATCam |
20100620 | 55367.82 | +12.9 | 18.261(0.041) | 17.701(0.033) | 19.233(0.148) | 17.700(0.040) | 17.442(0.037) | 17.378(0.068) | EM01 |
20100621 | 55368.79 | +13.9 | 18.325(0.051) | 17.752(0.025) | 19.186(0.109) | 17.650(0.049) | 17.550(0.046) | 17.432(0.072) | EM01 |
20100623 | 55370.80 | +15.9 | 18.367(0.096) | 17.797(0.090) | – | 17.665(0.048) | 17.419(0.072) | 17.313(0.088) | EM01 |
20100623 | 55371.41 | +16.5 | 18.422(0.022) | 17.850(0.033) | 19.322(0.137) | 17.687(0.049) | 17.550(0.039) | 17.428(0.056) | RATCam |
20100625 | 55373.41 | +18.5 | 18.449(0.039) | 17.907(0.036) | 19.405(0.160) | 17.619(0.058) | 17.504(0.039) | 17.445(0.058) | RATCam |
20100626 | 55373.80 | +18.9 | 18.468(0.089) | 17.810(0.049) | – | 17.667(0.029) | 17.574(0.046) | 17.395(0.074) | EM01 |
20100627 | 55374.80 | +19.9 | 18.489(0.054) | 17.930(0.044) | – | 17.854(0.047) | 17.637(0.043) | 17.374(0.073) | EM01 |
20100628 | 55375.79 | +19.9 | – | – | – | – | – | 17.465(0.174) | EM01 |
20100628 | 55376.39 | +21.5 | 18.699(0.052) | 17.934(0.019) | 19.612(0.123) | 17.828(0.012) | 17.558(0.044) | 17.473(0.062) | RATCam |
20100629 | 55377.42 | +22.5 | 18.658(0.030) | 17.922(0.027) | 19.559(0.130) | 17.799(0.010) | 17.553(0.027) | 17.466(0.115) | RATCam |
20101117 | 55517.18 | +162.3 | 22.555(0.101) | 22.019(0.040) | – | 21.461(0.066) | 20.618(0.053) | – | LRS |
20101213 | 55543.08 | +188.2 | – | 22.057(0.116) | – | 21.485(0.132) | 20.679(0.075) | – | LRS |
20101231 | 55561.20 | +206.3 | – | 22.053(0.149) | – | 21.494(0.101) | 20.721(0.125) | – | LRS |
20110105 | 55566.14 | +211.3 | – | – | – | 21.542(0.036) | – | – | LRS |
20111228 | 55923.11 | +568.2 | > 23.0 | > 22.9 | – | > 22.8 | – | – | AFOSC |
Notes.a Phases are relative to the r-band maximum light: MJD=55354.9.
b Johnson-Cousins R and I filter data were converted to Sloan r and i band magnitudes respectively, following the relations of Jordi et al. (2006)
c Unfiltered data obtained by amateur astronomers, calibrated to Sloan r-band magnitudes.
1 This approximation is based on the similar throughputs between wide filters F555W/F814W and V/I. Original data published by Berger (2010), and reported to Johnson-Cousins V and I (I> 24.9 mag) magnitudes.
2 Amateur data (K. Itagaki) scaled to r band.
3 Bright Supernova website (http://www.rochesterastronomy.org/sn2010/index.html#2010dn; Observation: J. Nicolas).
4 Bright Supernova website (http://www.rochesterastronomy.org/sn2010/index.html#2010dn; Observation: J. Brimacombe).
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