X-ray source | Expecteda | Candidatesb | |||||||||
CMaX | RA | Dec | Err | Cnts/ks | S/N | log![]() |
J | R | Optical | Near-IR | ![]() |
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 ![]() |
17N | 07:00:19 | -11:22:10 | 9 | 0.38 | 1.7 | 29.69 | 14.0 | 16.5 | 4 | 4 | 0.6 ![]() |
17S | 07:00:20 | -11:23:20 | 9 | 1.31 | 4.3 | 30.23 | 12.3 | 14.0 | 12 | 5 | 0.6 ![]() |
37 | 07:01:25 | -11:08:50 | 15 | 2.1 | 5.3 | 30.44 | 11.7 | 13.1 | 15 | 5 | 0.4 ![]() |
42 | 07:01:34 | -11:11:16 | 10 | 1.8 | 4.5 | 30.37 | 11.9 | 13.3 | 32 | 9 | 0.4 ![]() |
55S | 07:02:07 | -11:17:11 | 30 | 0.59 | 2.0 | 29.88 | 13.4 | 15.6 | 5 | 3 | ![]() |
55N | 07:02:08 | -11:16:15 | 30 | 0.72 | 2.6 | 29.97 | 13.1 | 15.2 | 2 | 1 | ![]() |
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 mag.
and
mag.; (b) (less than
50% of the candidates have near-IR counterpart).
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