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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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