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Table 2.

NIR photometry of the local sequences for SNhunt120 in the “standard” system.

ID α(2000) δ(2000) Y N Jrc2 N H N
101 223.4504 3.549965 13.60(01) 4 13.40(34) 5 12.73(03) 5
102 223.4811 3.582550 13.65(02) 5 13.41(03) 6 13.07(02) 6
103 223.4913 3.578437 15.10(02) 5 14.84(03) 6 14.47(03) 6
104 223.4615 3.557310 15.73(04) 5 15.25(04) 6 14.57(04) 6
105 223.4739 3.598759 15.66(04) 1 15.52(03) 2 15.23(06) 1
106 223.4524 3.570402 16.97(10) 4 16.37(15) 5 15.76(10) 5
107 223.4747 3.582985 17.47(21) 3 17.13(20) 3 16.53(19) 3

Notes. Values in parenthesis are 1σ uncertainties and correspond to an rms of the instrumental errors of the photometry obtained over the number of photometric nights N that standard star fields were observed.

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