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Table 2

X-ray sources identified with possible new cluster candidates.

LOX 2MASS Va Ra Ia J H Ks log LXb log LX/Lbolc Massc
(mag) (mag) (mag) (mag) (mag) (mag) (erg s-1) (M)

4 J05341833+0952376 15.09 14.37 13.66 12.72 12.21 12.02 29.80  −3.25 0.88
8 J05342809+0948476 17.42 16.16 14.80 13.32 12.59 12.40 29.78  −2.89 0.35
34 J05345260+0955500 ... 17.11* 14.89* 13.41 12.56 12.16 29.23  −3.41 0.33
39 J05345564+0957581 ... 17.25* 15.22* 13.71 12.96 12.73 28.93  −3.72 0.31
52 J05350064+0951510 ... 14.84* 13.74* 12.83 12.11 11.89 29.28  −3.79 0.48
56 J05350309+0956162 ... ... ... 12.69 12.04 11.77 29.65  −3.35 0.52
58 J05350356+0950531 ... 16.74* 15.04* 14.02 13.43 13.08 29.36  −3.27 0.27
59 J05350496+0956561 ... ... ... 13.22 12.52 12.28 29.33  −3.39 0.33
60 J05350528+0955149 ... ... ... 12.50 11.75 11.52 30.11  −2.97 0.59
69 J05350794+0950545 17.13 15.85 14.44 12.95 12.25 12.02 29.27  −3.55 0.35
76 J05351006+0950328 16.93 15.84 14.57 13.23 12.50 12.27 29.62  −3.13 0.38
79 J05351205+0955218 ... ... ... 13.44 12.77 12.52 30.10  −2.48 0.25
83 J05351456+0950026 17.00 15.85 14.52 13.06 12.32 12.06 29.34  −3.44 0.37
86 J05351606+0953374 ... 15.99* 14.36* 12.97 12.20 12.00 29.69  −3.20 0.31
92 J05351794+0954167 ... 15.54* 14.04* 12.65 11.88 11.65 29.79  −3.20 0.34
96 J05351857+0944058 16.83 15.78 14.47 13.02 12.31 12.06 29.55  −3.24 0.38
98 J05351857+0944058 11.85 11.29 10.77 9.89 9.38 9.14 31.04*  −3.20 1.98
107 J05352135+0954549 ... 15.91* 14.54* 13.29 12.59 12.38 28.81  −3.96 0.36
109 J05352216+0953586 17.07 15.82 14.53 13.08 12.38 12.14 29.83*  −2.94 0.38
112 J05352320+0952190 ... 17.37* 15.66* 14.26 13.55 13.28 28.48  −4.02 0.16
121 J05352846+1002275 17.18 15.97 14.58 13.15 12.45 12.16 28.99  −3.77 0.36
123 J05352920+0946317 14.78 14.05 13.37 12.31 11.69 11.56 29.73  −3.44 0.93
150 J05354495+0955190 ... ... ... ... 13.95 13.70 29.36d  −2.67 0.12
" J05354519+0955203 ... ... ... ... 13.71 13.44 29.36d  −2.78 0.14

Notes. 

(a)

Optical photometry from Dolan & Mathieu (2002), except for the values marked with an asterisk that are photographic magnitudes from the USNO-B1.0 or GSC2.3 catalogues.

(b)

X-ray luminosity in the 0.3 − 7.8 keV band assuming d = 400 pc. Values marked by an asterisk are derived from the spectral fits.

(c)

For stars with optical photometry, Lbol and masses were derived from the optical colours; for the others, they were computed from the J or Ks magnitudes for an age of 5 Myr.

(d)

The X-ray luminosity has been equally divided between the two stars (see text).

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