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Table A.2.
NIR photometry of the local sequences for SN 2013L in the standard system.
| ID | α (2000) | δ (2000) | Y | J | H |
|---|---|---|---|---|---|
| 101 | 11:45:38.03 | −50:34:20.8 | 11.583(016) | 11.414(017) | 11.078(018) |
| 102 | 11:45:27.47 | −50:34:29.0 | 13.217(011) | 12.829(003) | 12.332(024) |
| 103 | 11:45:36.91 | −50:36:11.3 | 14.119(011) | 13.753(009) | 13.317(012) |
| 104 | 11:45:37.61 | −50:34:49.5 | 14.205(018) | 13.970(005) | 13.701(032) |
| 105 | 11:45:19.92 | −50:36:31.8 | 14.224(010) | 13.835(003) | 13.318(026) |
| 106 | 11:45:30.63 | −50:35:38.9 | 14.386(020) | 14.105(006) | 13.760(038) |
| 107 | 11:45:26.68 | −50:34:55.4 | 14.549(008) | 14.225(009) | 13.860(030) |
| 108 | 11:45:34.50 | −50:36:50.5 | 14.645(013) | 14.371(004) | 14.078(026) |
| 109 | 11:45:31.15 | −50:35:24.9 | 14.784(011) | 14.455(011) | 14.050(044) |
| 110 | 11:45:34.94 | −50:35:52.6 | 14.972(015) | 14.716(011) | 14.459(051) |
| 111 | 11:45:24.04 | −50:37:18.4 | 15.036(024) | 14.582(030) | 13.899(019) |
| 112 | 11:45:35.32 | −50:36:02.4 | 15.486(040) | 15.168(022) | 14.834(075) |
| 113 | 11:45:29.55 | −50:35:13.7 | 15.457(021) | 15.311(031) | 15.135(063) |
| 114 | 11:45:35.20 | −50:34:46.9 | 15.619(036) | 15.326(016) | 14.967(042) |
| 115 | 11:45:36.77 | −50:34:58.7 | 15.628(032) | 15.251(029) | 14.793(043) |
| 116 | 11:45:27.75 | −50:37:16.2 | 15.684(026) | 15.379(034) | 14.874(054) |
| 117 | 11:45:28.67 | −50:36:16.8 | 15.701(026) | 15.373(020) | 15.017(024) |
| 118 | 11:45:24.91 | −50:34:30.9 | 15.770(032) | 15.459(003) | 15.074(034) |
| 119 | 11:45:39.29 | −50:36:46.4 | 15.843(011) | 15.405(035) | 14.918(053) |
| 120 | 11:45:21.80 | −50:35:09.1 | 15.867(034) | 15.505(004) | 15.142(036) |
| 121 | 11:45:30.05 | −50:36:28.7 | 15.827(016) | 15.313(019) | 14.725(040) |
| 122 | 11:45:35.90 | −50:35:10.9 | 15.899(032) | 15.448(017) | 14.885(026) |
| 123 | 11:45:24.27 | −50:35:24.5 | 15.868(018) | 15.349(015) | 14.781(051) |
| 124 | 11:45:24.36 | −50:36:09.0 | 16.670(090) | 16.270(017) | 15.924(127) |
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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