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Table A.2.
Calibration stars used for photometry in Sloan bands (AB) and Johnson/Cousins (Vega), as indicated in Fig. A.1.
| Star | u | g | r | i | z |
|---|---|---|---|---|---|
| 1 | 18.40 ± 0.02 | 17.07 ± 0.01 | 16.53 ± 0.01 | 16.33 ± 0.01 | 16.24 ± 0.01 |
| 2 | 18.94 ± 0.02 | 17.47 ± 0.01 | 16.93 ± 0.01 | 16.73 ± 0.01 | 16.62 ± 0.01 |
| 3 | 21.20 ± 0.11 | 19.48 ± 0.01 | 18.82 ± 0.01 | 18.56 ± 0.01 | 18.42 ± 0.03 |
| 4 | 17.35 ± 0.01 | 15.82 ± 0.01 | 15.27 ± 0.01 | 15.09 ± 0.01 | 15.00 ± 0.01 |
| 5 | 20.99 ± 0.09 | 19.36 ± 0.01 | 18.74 ± 0.01 | 18.49 ± 0.01 | 18.31 ± 0.03 |
| 6 | — | 20.80 ± 0.04 | 19.21 ± 0.02 | 18.65 ± 0.01 | 18.29 ± 0.05 |
| 7 | 21.63 ± 0.15 | 19.15 ± 0.01 | 17.82 ± 0.01 | 17.27 ± 0.01 | 16.97 ± 0.01 |
| 8 | 22.06 ± 0.21 | 20.16 ± 0.02 | 19.35 ± 0.01 | 18.98 ± 0.01 | 18.80 ± 0.04 |
| 9 | 21.13 ± 0.10 | 19.87 ± 0.02 | 19.54 ± 0.02 | 19.33 ± 0.02 | 19.34 ± 0.07 |
| 10 | – | – | 22.69 ± 0.20 | 21.60 ± 0.11 | – |
| 11 | – | 23.79 ± 0.33 | 22.27 ± 0.13 | 21.09 ± 0.07 | 20.95 ± 0.28 |
| 12 | 21.78 ± 0.17 | 19.01 ± 0.01 | 17.62 ± 0.01 | 16.91 ± 0.01 | 16.67 ± 0.01 |
| 13 | 20.82 ± 0.08 | 18.31 ± 0.01 | 17.07 ± 0.01 | 16.59 ± 0.01 | 16.31 ± 0.01 |
| 14 | 20.15 ± 0.05 | 19.00 ± 0.01 | 18.58 ± 0.01 | 18.37 ± 0.01 | 18.35 ± 0.03 |
| 15 | 19.74 ± 0.04 | 18.34 ± 0.01 | 17.77 ± 0.01 | 17.54 ± 0.01 | 17.38 ± 0.02 |
| 16 | 19.51 ± 0.03 | 18.52 ± 0.01 | 18.11 ± 0.01 | 17.92 ± 0.01 | 17.84 ± 0.02 |
| 17 | 17.88 ± 0.01 | 16.54 ± 0.01 | 16.06 ± 0.01 | 15.76 ± 0.01 | 15.79 ± 0.01 |
| 18 | – | 20.97 ± 0.03 | 19.62 ± 0.02 | 18.94 ± 0.01 | 18.68 ± 0.04 |
| 19 | 18.65 ± 0.02 | 17.54 ± 0.01 | 17.13 ± 0.01 | 16.97 ± 0.01 | 16.88 ± 0.01 |
| 20 | 20.21 ± 0.05 | 18.95 ± 0.01 | 18.54 ± 0.01 | 18.37 ± 0.01 | 18.33 ± 0.03 |
| Star | U | B | V | RC | IC |
| 1 | 17.65 ± 0.04 | 17.49 ± 0.03 | 16.74 ± 0.02 | 16.30 ± 0.03 | 15.89 ± 0.02 |
| 2 | 18.16 ± 0.04 | 17.89 ± 0.03 | 17.14 ± 0.02 | 16.70 ± 0.03 | 16.29 ± 0.02 |
| 3 | 21.41 ± 0.12 | 19.95 ± 0.03 | 19.08 ± 0.02 | 18.58 ± 0.03 | 18.11 ± 0.03 |
| 4 | 16.56 ± 0.04 | 16.24 ± 0.03 | 15.49 ± 0.02 | 15.07 ± 0.03 | 14.68 ± 0.02 |
| 5 | 20.30 ± 0.10 | 19.81 ± 0.03 | 18.98 ± 0.02 | 18.49 ± 0.03 | 18.03 ± 0.03 |
| 7 | 20.93 ± 0.16 | 19.87 ± 0.03 | 18.36 ± 0.02 | 17.54 ± 0.03 | 16.77 ± 0.02 |
| 8 | 21.29 ± 0.21 | 20.69 ± 0.04 | 19.67 ± 0.02 | 19.05 ± 0.03 | 18.47 ± 0.04 |
| 9 | 21.31 ± 0.11 | 20.21 ± 0.04 | 19.67 ± 0.02 | 19.22 ± 0.04 | 18.80 ± 0.07 |
| 12 | 21.04 ± 0.17 | 19.76 ± 0.03 | 18.18 ± 0.02 | 17.19 ± 0.03 | 16.27 ± 0.02 |
| 13 | 20.08 ± 0.09 | 19.00 ± 0.03 | 17.57 ± 0.02 | 16.83 ± 0.03 | 16.14 ± 0.02 |
| 14 | 19.39 ± 0.06 | 19.37 ± 0.03 | 18.74 ± 0.02 | 18.29 ± 0.03 | 17.87 ± 0.03 |
| 15 | 18.98 ± 0.06 | 18.77 ± 0.03 | 17.99 ± 0.02 | 17.24 ± 0.03 | 17.08 ± 0.02 |
| 16 | 18.74 ± 0.05 | 18.86 ± 0.02 | 18.27 ± 0.02 | 17.88 ± 0.02 | 17.48 ± 0.02 |
| 17 | 17.10 ± 0.04 | 16.94 ± 0.03 | 16.25 ± 0.02 | 15.70 ± 0.03 | 15.19 ± 0.02 |
| 19 | 17.85 ± 0.04 | 17.88 ± 0.03 | 17.29 ± 0.02 | 16.93 ± 0.03 | 16.56 ± 0.02 |
| 20 | 19.42 ± 0.06 | 19.32 ± 0.02 | 18.70 ± 0.02 | 18.29 ± 0.02 | 17.91 ± 0.03 |
Notes.The transformation from Sloan to Johnson/Cousins was done using the Jester et al. (2005) transformations.
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