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Table 2

Optical and NIR photometry of the local sequence of SN 2012Z in the natural system.

u N g N r N i N B N V N Y N J N H N
STAR α (2000) δ (2000) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag)

001 03:22:15.58 –15:19:11.93 15.026(007) 17 ··· ··· ··· ··· ··· ··· 13.339(005) 7 ··· ··· ··· ··· ··· ··· ··· ···
002 03:22:19.50 –15:19:19.63 14.038(006) 18 ··· ··· ··· ··· ··· ··· 13.282(005) 7 12.762(011) 1 ··· ··· ··· ··· ··· ···
003 03:22:00.97 –15:19:28.24 14.358(006) 18 ··· ··· ··· ··· ··· ··· 13.399(005) 8 12.759(011) 1 ··· ··· ··· ··· ··· ···
004 03:21:52.18 –15:20:52.44 17.045(010) 19 16.002(003) 22 15.636(003) 20 15.501(003) 25 16.304(003) 26 15.791(003) 28 ··· ··· ··· ··· ··· ···
005 03:22:05.62 –15:22:34.86 17.007(010) 19 16.022(003) 22 15.618(003) 20 15.471(003) 25 16.330(003) 27 15.795(003) 29 ··· ··· ··· ··· ··· ···
006 03:21:54.34 –15:21:12.06 17.220(011) 19 16.101(003) 22 15.648(003) 20 15.477(003) 25 16.435(003) 27 15.849(003) 29 ··· ··· ··· ··· ··· ···
007 03:22:18.71 –15:19:27.70 19.076(044) 10 16.957(004) 19 16.159(004) 17 15.844(004) 20 17.441(007) 22 16.565(004) 23 ··· ··· ··· ··· ··· ···
008 03:22:09.62 –15:22:13.87 18.311(020) 18 17.188(004) 22 16.780(005) 20 16.616(005) 25 17.532(006) 27 16.965(004) 29 ··· ··· ··· ··· ··· ···
009 03:22:18.09 –15:24:01.51 ··· ··· 18.486(010) 22 17.342(006) 20 16.861(006) 25 18.905(018) 20 17.920(008) 29 ··· ··· ··· ··· ··· ···
010 03:21:53.30 –15:27:14.29 ··· ··· 19.155(024) 11 17.840(012) 12 16.165(006) 15 19.778(071) 5 18.510(018) 17 ··· ··· ··· ··· ··· ···
011 03:22:12.29 –15:19:41.63 ··· ··· 19.133(019) 17 17.742(009) 18 16.700(005) 22 19.788(047) 9 18.442(013) 28 ··· ··· ··· ··· ··· ···
012 03:22:16.89 –15:20:44.88 18.917(082) 1 18.880(014) 21 18.060(011) 20 17.628(010) 25 18.962(024) 14 18.463(014) 29 ··· ··· ··· ··· ··· ···
013 03:21:48.55 –15:21:14.36 19.452(094) 3 18.817(018) 13 18.476(019) 14 18.291(023) 16 18.755(022) 14 18.587(017) 22 ··· ··· ··· ··· ··· ···
014 03:21:52.45 –15:27:02.48 18.958(048) 7 18.991(017) 16 18.666(019) 17 18.674(031) 18 18.970(025) 13 18.881(023) 20 ··· ··· ··· ··· ··· ···
015 03:22:22.44 –15:20:44.09 ··· ··· 19.444(024) 16 18.628(017) 19 18.263(018) 24 19.445(044) 8 18.885(022) 20 ··· ··· ··· ··· ··· ···
016 03:21:55.41 –15:20:24.11 ··· ··· 20.111(044) 12 18.848(021) 19 17.568(010) 25 20.147(104) 3 19.480(036) 15 ··· ··· ··· ··· ··· ···
017 03:22:14.78 –15:27:04.36 ··· ··· 20.372(097) 3 19.082(032) 11 18.222(020) 17 ··· ··· 19.656(059) 7 ··· ··· ··· ··· ··· ···
018 03:22:05.60 –15:22:35.06 ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· 14.808(016) 4 14.572(017) 5 14.246(014) 5
019 03:22:03.04 –15:22:27.83 ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· 16.431(024) 4 16.035(028) 5 15.384(023) 5
020 03:22:09.59 –15:22:13.71 ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· 15.973(020) 4 15.708(024) 5 15.398(022) 5
021 03:22:04.73 –15:23:44.15 ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· 16.357(033) 4 15.901(032) 5 15.245(029) 5
022 03:22:01.66 –15:22:30.86 ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· 18.399(096) 2 ··· ··· ··· ···
023 03:22:05.94 –15:24:38.59 ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· ··· 17.229(100) 1 16.854(104) 1 16.383(119) 1

Notes. Uncertainties given in parentheses in thousandths of a magnitude correspond to an rms of the magnitudes obtained on photometric nights.

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