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Table 7:

2MASS sources associated with the centimeter and/or millimeter emission toward the star-forming region IRAS 00117+6412.
  2MASS Position       J-H $H-K_{{\rm S}}$  
Source Identification $\alpha (\rm J2000)$ $\delta (\rm J2000)$ J H $K_{{\rm S}}$ colora colora IR $_{\rm excess}$b

UCH II 		00142828+6428471 00 14 28.29 64 28 47.19 $14.94\pm0.08$ $13.28\pm0.07$ $12.14\pm0.05$ 1.66 1.14 +0.18
MM1 00142616+6428444 00 14 26.16 64 28 44.44 $15.49\pm0.07$ $13.58\pm0.06$ $12.22\pm0.04$ 1.91 1.37 +0.27
2M0014256 00142558+6428416 00 14 25.59 64 28 41.70 $16.71\pm0.14$ $14.35\pm0.05$ $13.27\pm0.04$ 2.36 1.09 -0.27

Notes. (a) Uncertainties in the colors are typically $\sim $0.09 mag. (b) The infrared excess is measured as the difference between the $(H-K_{{\rm S}})$ color and the $(H-K_{{\rm S}})$ color corresponding to a reddened main-sequence star (following the reddening law of Rieke & Lebofsky 1985), i.e., ${\rm IR_{excess}}=(H-K_{{\rm S}})-0.576\times(J-K_{{\rm S}})$.


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