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Table A.3

Local sequence stars used to calibrate SN 2015H NTT photometry.

No. RA Dec V J H K
(mag) (mag) (mag) (mag)

3 10:54:48.88 –21:04:33.8 17.89(0.01) 14.77(0.03) 14.07(0.04) 13.91(0.05)
15 10:54:48.35 –21:04:59.1 18.14(0.02) 14.58(0.04) 13.93(0.04) 13.69(0.04)
16 10:54:45.45 –21:05:47.3 15.01(0.01) 13.41(0.03) 12.92(0.03) 12.92(0.03)
17 10:54:38.89 –21:04:33.8 17.35(0.01) 16.20(0.08) 15.80(0.14) 15.87(0.28)
18 10:54:35.85 –21:03:36.2 15.98(0.01) 14.70(0.04) 14.34(0.04) 14.20(0.07)

Notes. V-band magnitudes of sequence stars are derived from SDSS9 gr magnitudes, and shown to two decimal places in the AB system. IR magnitudes are taken from 2MASS Point Source Catalogue in the 2MASS natural system. 1σ uncertainties are given in parentheses.

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