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Table A.1.

Optical photometry of the local sequences for SN 2013L in the standard system.

ID α (2000) δ (2000) B V u g r i
1 176.372940 −50.566639 14.085(009) 13.564(012) 14.909(017) 13.779(008) 13.432(007) 13.320(010)
2 176.420593 −50.632069 15.631(022) 14.548(010) 17.259(081) 15.046(015) 14.197(009) 13.857(009)
3 176.448257 −50.577740 16.060(022) 15.407(018) 16.993(032) 15.694(016) 15.224(013) 15.057(013)
4 176.415695 −50.644630 16.866(036) 16.172(023) 17.808(068) 16.480(029) 15.967(018) 15.766(021)
5 176.474594 −50.619598 17.240(055) 16.431(030) 18.459(097) 16.781(026) 16.189(019) 15.972(015)
6 176.288162 −50.547031 17.699(083) 16.877(043) 19.023(131) 17.256(045) 16.607(035) 16.372(035)
7 176.435425 −50.628880 19.067(071) 17.724(059) 18.882(078) 18.358(066) 17.143(033) 16.646(038)
8 176.278427 −50.581089 18.180(025) 17.479(064) 19.078(107) 17.794(049) 17.252(033) 17.028(048)
9 176.351624 −50.602581 18.319(148) 17.706(079) 19.175(095) 18.030(056) 17.533(054) 17.314(043)
10 176.417496 −50.562401 18.988(050) 18.080(098) ... 18.515(055) 17.758(038) 17.467(071)
11 176.274002 −50.595940 17.639(103) 17.391(042) 18.770(060) 17.448(037) 17.415(065) 17.481(073)
12 176.376709 −50.653801 19.092(042) 18.114(105) 20.204(115) 18.582(096) 17.832(068) 17.550(083)
13 176.394547 −50.654530 19.970(038) 18.624(094) ... 19.203(106) 18.076(085) 17.601(058)
14 176.468704 −50.540169 19.102(075) 18.173(092) 20.451(194) 18.608(100) 17.842(060) 17.585(066)
15 176.309906 −50.574009 ... 19.697(077) ... 20.394(049) 19.003(092) 17.559(076)
17 176.342255 −50.543720 16.666(035) 15.964(019) 17.668(062) 16.267(027) 15.756(016) 15.563(015)
18 176.293945 −50.667351 15.999(022) 15.157(014) 17.388(019) 15.532(019) 14.892(013) 14.690(012)
19 176.322266 −50.618359 17.310(040) 16.521(036) 18.468(103) 16.868(026) 16.272(019) 16.062(023)
20 176.484634 −50.526569 ... ... ... 20.639(148) 19.856(096) 18.523(074)
21 176.406937 −50.592899 18.120(089) 17.457(076) 19.107(135) 17.749(043) 17.238(044) 17.061(041)

Notes. Values in parenthesis are 1-σ uncertainties and correspond to a root mean square (rms) of the instrumental errors of the photometry obtained over a minimum of three photometric nights.

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