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Table E.6.

Photometry for the NGC 1960 members retrieved from the literature.

Object Rc Ic g r i rIPHAS iIPHAS HαIPHAS J
[mag] [mag] [mag] [mag] [mag] [mag] [mag] [mag] [mag]
876 17.34 0.13 16.508 0.008 18.87 0.15 (17.639 0.14) (16.922 0.009) 17.534 0.050 16.638 0.051 17.151 0.051 15.211 0.050
827 17.50 0.13 16.583 0.008 19.28 0.15 (17.928 0.14) (17.086 0.009) 17.838 0.051 16.897 0.051 17.344 0.051 15.434 0.051
829 17.46 0.13 16.591 0.008 19.20 0.15 (17.841 0.14) (17.063 0.009) 17.542 0.050 16.728 0.051 17.119 0.051 15.323 0.051
1056 18.03 0.13 16.979 0.008 19.88 0.16 18.462 0.15 17.496 0.009 18.298 0.051 17.180 0.051 17.789 0.052 15.918 0.054
1269 18.43 0.13 17.284 0.009 20.42 0.17 18.962 0.15 17.848 0.010 18.832 0.052 17.592 0.053 18.282 0.055 16.031 0.052
1291 18.41 0.13 17.181 0.009 20.29 0.17 18.894 0.15 17.736 0.010 18.821 0.053 17.500 0.053 18.147 0.054 15.879 0.052
1042 17.66 0.16 16.729 0.012 - - - - - - 17.841 0.050 16.895 0.051 17.401 0.051 15.547 0.052
1833 18.57 0.13 17.357 0.009 20.54 0.17 19.107 0.15 17.919 0.010 19.075 0.054 17.809 0.054 18.542 0.060 16.043 0.057
1859 19.40 0.15 17.863 0.010 21.24 0.23 19.794 0.17 18.371 0.010 19.425 0.058 17.989 0.057 18.814 0.064 16.469 0.056
1860 19.38 0.14 17.853 0.010 21.33 0.31 19.949 0.29 18.490 0.020 19.485 0.059 17.928 0.056 18.763 0.063 16.192 0.054
1878 19.24 0.14 17.712 0.010 21.33 0.20 19.803 0.16 18.306 0.010 19.722 0.064 18.042 0.057 18.958 0.067 16.171 0.052
1545 18.83 0.13 17.509 0.009 20.67 0.18 (19.278 0.15) (18.047 0.010) 19.186 0.055 17.735 0.054 18.486 0.058 16.119 0.052
1540 19.23 0.14 17.678 0.010 21.13 0.19 19.762 0.16 18.269 0.010 19.760 0.033 17.909 0.056 18.710 0.061 16.198 0.052
2171 19.81 0.16 18.191 0.011 22.50 0.56 20.538 0.37 18.999 0.024 20.351 0.079 18.540 0.065 19.529 0.087 16.815 0.057
1871 19.56 0.15 18.015 0.011 21.56 0.22 20.098 0.17 18.602 0.011 20.102 0.075 18.342 0.062 19.261 0.078 16.664 0.063
2188 19.76 0.16 18.179 0.011 (21.72 0.24) 20.336 0.18 (18.822 0.011) 19.971 0.071 18.510 0.066 19.199 0.075 16.654 0.063
2249 20.01 0.17 18.270 0.012 22.18 0.28 20.605 0.18 18.928 0.011 19.966 0.087 18.450 0.078 19.936 0.169 16.753 0.062
2173 19.95 0.16 18.334 0.012 22.03 0.26 20.573 0.18 18.952 0.011 20.667 0.088 18.791 0.068 19.986 0.113 16.703 0.063
2696 20.27 0.18 18.584 0.014 22.38 0.30 20.942 0.19 19.240 0.012 21.385 0.184 18.966 0.084 20.407 0.178 17.106 0.062
2214 19.80 0.16 18.213 0.012 21.87 0.24 20.424 0.17 18.856 0.011 20.460 0.093 18.514 0.066 19.493 0.089 16.855 0.058
2663 20.11 0.17 18.412 0.013 22.13 0.27 20.741 0.19 19.054 0.012 20.627 0.101 18.852 0.078 20.122 0.141 17.087 0.075
2703 20.18 0.17 18.490 0.013 22.31 0.28 20.726 0.18 19.097 0.012 20.860 0.124 19.005 0.084 20.061 0.134 17.041 0.061
2672 20.39 0.18 18.658 0.014 22.40 0.40 21.063 0.35 19.305 0.022 20.863 0.120 18.985 0.085 20.106 0.139 17.174 0.065
3081 20.42 0.31 18.711 0.021 22.59 0.40 21.241 0.25 19.380 0.015 20.464 0.101 18.952 0.089 19.888 0.133 17.189 0.083
3150 20.67 0.20 18.843 0.016 22.77 0.35 21.407 0.22 19.532 0.013 21.809 0.266 19.245 0.100 20.970 0.292 17.353 0.067
3080 20.69 0.20 18.795 0.016 22.97 0.39 21.333 0.22 19.442 0.013 20.488 0.106 19.215 0.111 20.149 0.174 - -
3590 20.97 0.22 19.107 0.019 23.56 0.49 21.751 0.26 19.779 0.015 - - 19.902 0.159 21.048 0.304 17.551 0.082
3073 20.58 0.20 18.785 0.016 22.61 0.32 21.289 0.22 19.460 0.013 (22.952 0.674) 19.022 0.082 (21.819 0.591) 17.884 0.139
3028 20.97 0.22 19.060 0.019 23.43 0.46 21.675 0.24 19.754 0.014 21.813 0.240 19.681 0.130 20.768 0.229 17.606 0.089
3612 21.06 0.24 19.152 0.021 23.35 0.45 21.618 0.24 19.822 0.015 - - 19.892 0.162 - - 17.745 0.085
3596 21.08 0.23 19.185 0.020 23.17 0.40 21.651 0.24 19.895 0.015 22.251 0.395 19.896 0.166 20.652 0.221 17.982 0.109
4165 21.46 0.27 19.469 0.025 23.89 0.54 22.257 0.30 20.213 0.018 - - 20.938 0.482 - - 17.978 0.102

Note: The photometric values in brackets correspond to cases where we encountered problems in the SED reconstruction procedure.

References: RcIc are taken from Jeffries et al. (2013); gri from Bell et al. (2013); riHαIPHAS from Barentsen et al. (2014); J from Galindo-Guil et al. (in prep).

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