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Table A.3

Objects with questioned membership from the CFHT UV-census.

Mon-ID RA Dec u g r i Membership criteria

Mon-000003 100.43878 9.78583 20.460 18.204 16.924 16.206 P, X
Mon-000004 100.56094 9.84104 17.808 15.998 15.075 14.594 P, RV
Mon-000025 100.51118 9.97441 18.025 16.134 15.193 14.690 P, RV
Mon-000031 100.55471 9.76763 17.801 16.118 15.307 14.888 P, RV
Mon-000387 100.45535 9.68496 20.530 18.408 17.273 16.681 X
Mon-000414 100.55863 9.59579 18.446 16.440 15.431 14.944 P, RV
Mon-000593* 100.25704 9.35157 17.793 15.822 15.077 14.836 P, RV
Mon-000600* 100.20549 9.98095 22.567 19.684 18.106 17.212 X
Mon-000696* 100.33708 9.57170 20.309 19.512 19.589 18.516 h
Mon-000820 100.48089 9.50528 19.538 17.513 16.490 15.902 X
Mon-000944 100.45795 9.68479 20.258 18.274 17.185 16.629 X
Mon-000946* 100.20165 9.99424 21.252 18.810 17.472 16.715 II
Mon-000966 100.19639 9.30923 17.729 15.882 14.942 14.415 P, RV
Mon-000976 100.43282 9.15588 21.325 19.108 17.798 17.058 X
Mon-000983 100.24170 9.30085 16.047 14.663 14.206 14.042 RV
Mon-000988 100.08816 9.98401 20.823 18.249 16.758 15.930 P, RV
Mon-001043* 100.06439 9.71678 21.746 19.149 17.695 16.854 P, II/III
Mon-001046 99.98493 9.72542 15.811 14.455 14.048 13.881 RV
Mon-001086 99.88986 9.86127 18.279 16.524 15.639 15.144 P, RV
Mon-001192 100.16157 9.36066 17.954 15.866 15.079 14.799 RV
Mon-001207 99.98039 9.98644 21.113 18.345 16.911 16.009 h
Mon-001283* 99.86101 9.51055 21.364 18.750 17.590 17.012 RV
Mon-001289 99.85268 9.37588 16.778 15.082 14.379 14.084 P, RV
Mon-001293 99.89724 9.54233 18.331 16.315 15.239 14.681 P, RV
Mon-001311 99.81513 9.65357 18.014 16.134 15.181 14.684 P, RV
Mon-001393 100.55236 9.98531 17.072 15.373 14.609 14.195 P, RV
Mon-006019* 100.14231 9.42022 19.511 17.507 16.217 15.507 P
Mon-007454 100.12886 10.08013 17.799 16.099 15.494 15.140 P

Notes. Membership criteria, in the literature, for the listed objects: P = photometric member (i.e., located on a cluster sequence in the R vs. RI diagram); X = X-ray emitter, from Sung et al. (2009); RV = radial velocity member, from Fűrész et al. (2006); h = Hα emission candidate, from Sung et al. (2009); II = Class II object, from Sung et al. (2009); II/III = Class II/III object, from Sung et al. (2009).

(*)

More uncertain cases.

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