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Table A.4

Local griz sequence stars use to calibrate LSQ13fn photometry.

# RA Dec g r i z

1 11:51:17.775 29:34:54.09 18.64 (0.04) 17.26 (0.04) 16.29 (0.03) 15.61 (0.04)
2 11:51:21.373 29:35:17.58 14.86 (0.03) 14.16 (0.02) 13.91 (0.02) 13.78 (0.02)
3 11:51:22.206 29:35:25.91 18.08 (0.02) 17.17 (0.03) 16.83 (0.02) 16.60 (0.03)
4 11:51:10.039 29:35:06.90 18.83 (0.04) 18.05 (0.03) 17.78 (0.04) 17.68 (0.03)
5 11:51:21.139 29:36:38.81 18.74 (0.04) 17.09 (0.03) 16.27 (0.02) 15.65 (0.03)
6 11:51:25.397 29:37:43.70 18.16 (0.04) 16.55 (0.04) 15.68 (0.03) 15.06 (0.03)
7 11:51:24.406 29:37:59.94 18.28 (0.03) 17.71 (0.04) 17.55 (0.04) 17.39 (0.05)
8 11:51:21.321 29:37:53.01 17.13 (0.04) 15.75 (0.03) 15.20 (0.03) 14.79 (0.03)
9 11:51:21.954 29:38:12.99 16.96 (0.04) 16.16 (0.03) 15.85 (0.03) 15.67 (0.01)

Notes. Uncertainties are given in parentheses.

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