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Table 1.

Photometry of the local sequence for SNhunt120 in the “standard” system.

ID α (2000) δ (2000) B V u g r i
1 223.501175 3.554772
2 223.494568 3.512511
3 223.450409 3.549971
4 223.491287 3.578468 16.572(028) 16.018(011) 17.253(048) 16.239(009) 15.847(019) 15.692(010)
5 223.454926 3.543110 16.771(020) 16.082(012) 17.797(071) 16.387(010) 15.892(007) 15.716(010)
6 223.473694 3.598971 17.385(050) 16.734(025) 18.245(055) 17.016(035) 16.567(029) 16.392(021)
7 223.545074 3.513310 17.712(029) 17.034(024) 18.675(033) 17.374(035) 16.854(013) 16.661(024)
8 223.423279 3.524919 18.486(023) 17.988(049) 19.094(043) 18.198(036) 17.827(034) 17.709(060)
9 223.409164 3.544031 18.709(027) 18.131(044) 19.455(207) 18.315(119) 17.930(072) 17.795(068)
10 223.525085 3.558814 19.137(166) 18.274(018) 20.034(082) 18.703(032) 17.994(079) 17.723(096)
11 223.461456 3.557315 19.394(061) 17.967(060) 19.917(172) 18.701(003) 17.397(041) 16.743(016)
12 223.466751 3.512445 19.219(068) 18.595(080) 19.980(066) 18.800(085) 18.276(096) 18.154(070)
13 223.450058 3.525849 19.625(047) 18.460(053) 18.985(028) 17.875(043) 17.522(032)
14 223.413147 3.509561 19.529(075) 18.903(025) 19.950(072) 19.241(025) 18.724(024) 18.467(052)
15 223.500031 3.629244 19.735(062) 18.549(084) 19.149(033) 17.913(043) 17.394(027)
16 223.488373 3.505094 19.659(061) 18.660(035) 19.168(068) 18.195(060) 17.927(074)
17 223.537628 3.636855 19.683(100) 19.045(044) 20.249(094) 19.355(005) 18.847(103) 18.771(035)
18 223.432632 3.621403 19.990(188) 19.316(039) 20.400(132) 19.637(111) 19.189(035) 18.764(062)
19 223.469666 3.623828 19.806(138) 19.236(086) 19.574(057) 18.878(003) 18.537(061)
20 223.407272 3.620129 19.984(091) 19.721(097) 19.100(063) 20.079(100) 19.521(052) 19.187(014)
21 223.508453 3.619909 20.646(152) 19.390(189) 20.051(112) 18.770(084) 18.039(116)

Notes. Values in parenthesis are 1σ 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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