Table 7: Near-infrared photometry of a few new Praesepe candidates.
Object Teles. J H $K_{\rm s}$ z'-J $J-K_{\rm s}$ Phot. Prob.a

Prae J083850.6+192317b		 2MASS 16.37 $\pm$ 0.11 16.01 $\pm$ 0.18 15.40 $\pm$ 0.19 1.20 $\pm$ 0.23 0.97 $\pm$ 0.12 high/high
Prae J084051.2+191010c 2MASS 16.75 $\pm$ 0.15 15.76 $\pm$ 0.15 15.59 $\pm$ 0.23 1.00 $\pm$ 0.25 1.16 $\pm$ 0.27 low/high
WFC 24d TCS 17.71 $\pm$ 0.33     2.6 $\pm$ 0.4   high/high
Prae J084111.9+192043 WHT 19.85 $\pm$ 0.07 18.95 $\pm$ 0.11 18.28 $\pm$ 0.10 2.48 $\pm$ 0.21 1.57 $\pm$ 0.12 high/high
a Optical / near-infrared photometric cluster membership probability; b 2MASS J08385059+1923164; c 2MASS J08405122+1910106; d  $J = 17.99 \pm0.03$, $H = 17.30 \pm0.02$, $K = 16.78 \pm0.02$ (Chappelle et al. 2005).

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