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Table 1:

List of CMaX sources observed with Gemini.
  X-ray source Expecteda Candidatesb  
CMaX RA Dec Err Cnts/ks S/N log$L_{\rm X}$ J R Optical Near-IR $A_{\rm V}$
  J2000 J2000 ('')     (erg/s) (mag) (mag)     (mag)
15 07:00:15 -11:18:51 10 1.9 4.8 30.39 11.8 13.3 12 6 1.23 $\pm$ 0.03
17N 07:00:19 -11:22:10 9 0.38 1.7 29.69 14.0 16.5 4 4 0.6 $\pm$ 0.3
17S 07:00:20 -11:23:20 9 1.31 4.3 30.23 12.3 14.0 12 5 0.6 $\pm$ 0.3
37 07:01:25 -11:08:50 15 2.1 5.3 30.44 11.7 13.1 15 5 0.4 $\pm$ 0.6
42 07:01:34 -11:11:16 10 1.8 4.5 30.37 11.9 13.3 32 9 0.4 $\pm$ 0.6
55S 07:02:07 -11:17:11 30 0.59 2.0 29.88 13.4 15.6 5 3 $1.2\pm1.0$
55N 07:02:08 -11:16:15 30 0.72 2.6 29.97 13.1 15.2 2 1 $1.2\pm1.0$

Columns description: (1) CMaX number; (2, 3) coordinates; (4) diameter of the position error circle; (5, 6) count rate and respective signal-to-noise ratio; (7) X-ray luminosity; (8, 9) Statistically expected near-IR and optical magnitudes calculated by adopting the correlation logLX/absolute magnitude found for young stars (see Sect. 4.4); (10, 11) Number of possible optical counterparts within the X-ray contours, and number of corresponding objects found in the 2MASS catalogue; (12) adopted visual extinction based on a standard reddening law.
Notes: (a) The estimated errors are $\sigma_J= 1.2$ mag. and $\sigma_R= 1.4$ mag.; (b) (less than 50% of the candidates have near-IR counterpart).


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