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Table 5

The 9 Praesepe cluster candidates identified by Boudreault et al. (2010) that were rejected in this work by colour or brightness.

ID RA(J2000) Dec(J2000) i z Ic J Ks M Teff Jmodel
(mag) (mag) (mag) (mag) (mag) (M) (K) (mag)

005 8:41:08.50 +19:54:02.0 20.19 18.70 19.02 16.58 15.39 0.088 2636 17.06
007 8:39:39.56 +19:47:54.3 18.93 17.80 17.95 16.10 15.07 0.104 2860 16.58
009 8:39:55.84 +19:53:14.3 18.05 17.78 20.29 17.50 16.54 0.081 2520 17.32
018 8:39:42.79 +19:35:48.2 18.27 16.20 15.21 0.097 2782 16.78
022 8:41:04.20 +19:31:27.8 20.12 19.15 18.89 16.67 15.75 0.092 2702 16.97
901 8:39:59.45 +19:43:37.4 18.05 18.30 19.09 17.16 16.41 0.084 2574 17.20
902 8:39:23.72 +19:52:01.8 20.41 19.46 20.15 17.77 16.88 0.073 2348 17.72
903 8:40:00.20 +19:30:27.0 19.59 19.01 19.74 17.50 16.62 0.076 2409 17.57
914 8:38:52.02 +19:35:05.3 19.48 18.69 19.12 17.25 16.35 0.085 2591 17.16

Notes. The IDs in the first column are taken from Boudreault et al. (2010). The fourth object is not a point-like source in the LBT image, thus no optical photometry measurement is available.

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