Table 4
Spectral parameters of brighter sources.
| Source | CP / | CXOU J | Net Counts | Log NH | k T 1 | k T 2 | Log Ls | Log Lh | Log Lh,c | Log Lt | Log Lt,c | |||
| No. | IR class | (counts) | (cm-2) | (keV) | (keV) | (erg s-1) | (erg s-1) | (erg s-1) | (erg s-1) | (erg s-1) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | |||
|
|
||||||||||||||
| 1 | yes | 061147.81+180312.6 | 443.3 | 21.81 ± 0.15 | 0.7 ± 0.1 | – | 30.89 | 30.14 | 30.19 | 30.97 | 31.47 | |||
| 2 | no | 061154.83+180016.5 | 192.1 | 22.04 ± 0.46 | 15.0 ± 5.1 | – | 30.26 | 31.08 | 31.11 | 31.14 | 31.27 | |||
| 3 | yes | 061159.55+175802.9 | 159.6 | 22.38 ± 0.64 | 2.6 ± 1.2 | – | 30.21 | 30.96 | 31.05 | 31.03 | 31.40 | |||
| 5 | yes/III | 061206.65+180336.6 | 239.0 | 21.41 ± 0.16 | 0.5 ± 0.1 | – | 30.88 | 29.55 | 29.57 | 30.90 | 31.17 | |||
| 27 | yes | 061230.43+175506.8 | 81.8 | 20.48 ± 0.19 | 9.4 ± 9.9 | – | 30.23 | 30.53 | 30.53 | 30.70 | 30.71 | |||
| 30 | yes | 061230.98+180336.9 | 386.2 | 22.07 ± 0.13 | 15.0∗ | – | 30.62 | 31.46 | 31.49 | 31.52 | 31.65 | |||
| 32 | yes | 061231.17+180853.8 F | 99.5 | 21.96 ± 0.41 | 3.8 ± 2.3 | – | 30.28 | 30.78 | 30.81 | 30.90 | 31.09 | |||
| 97 | yes/III | 061244.17+175914.0 | 174.6 | 21.56 ± 0.26 | 0.6 ± 0.2 | 3.4 ± 1.6 | 30.57 | 30.45 | 30.46 | 30.81 | 31.02 | |||
| 102 | yes | 061244.76+175946.8 | 156.6 | 21.61 ± 0.15 | 3.1 ± 0.8 | – | 30.41 | 30.65 | 30.67 | 30.85 | 30.98 | |||
| 104 | yes | 061245.23+175810.3 F | 116.6 | 20.0∗ | 1.5 ± 0.2 | – | 30.45 | 30.06 | 30.06 | 30.60 | 30.61 | |||
| 113 | yes/III | 061246.71+175418.2 | 86.6 | 21.53 ± 0.23 | 0.7 ± 0.1 | – | 30.38 | 29.47 | 29.49 | 30.43 | 30.73 | |||
| 147 | yes/III | 061251.04+180644.1 | 141.8 | 20.00 ± 16.03 | 1.0 ± 0.1 | – | 30.69 | 29.66 | 29.66 | 30.73 | 30.74 | |||
| 183 | yes | 061253.48+175633.9 | 91.2 | 23.08 ± 3.43 | 54.2 ± 724 | – | 28.43 | 31.13 | 31.35 | 31.13 | 31.48 | |||
| 190 | yes | 061253.73+175724.7 | 373.2 | 22.99 ± 1.25 | 5.4 ± 1.2 | – | 29.51 | 31.64 | 31.88 | 31.65 | 32.11 | |||
| 209 | yes | 061254.33+175927.7 F | 86.5 | 22.86 ± 1.99 | 8.6 ± 10.8 | – | 29.13 | 30.99 | 31.16 | 31.00 | 31.35 | |||
| 230 | yes | 061255.04+175930.7 F | 250.5 | 22.30 ± 0.53 | 0.9 ± 0.4 | 8.7 ± 13.0 | 30.44 | 31.11 | 31.18 | 31.20 | 31.61 | |||
| 255 | yes/I | 061258.21+175848.1 | 91.7 | 22.34 ± 0.53 | 2.6 ± 0.9 | – | 30.00 | 30.70 | 30.79 | 30.78 | 31.14 | |||
| 333 | yes | 061312.58+180706.2 | 379.7 | 22.56 ± 0.46 | 7.9 ± 3.5 | – | 30.33 | 31.60 | 31.70 | 31.63 | 31.90 | |||
| 337 | no | 061316.04+175416.7 | 139.9 | 22.22 ± 0.42 | 3.9 ± 1.6 | – | 30.19 | 30.91 | 30.96 | 30.98 | 31.24 | |||
| 341 | yes | 061317.11+175344.9 F | 265.6 | 21.74 ± 0.17 | 5.0 ± 1.6 | – | 30.70 | 31.16 | 31.17 | 31.29 | 31.41 | |||
| 348 | yes/II | 061325.57+175230.5 | 163.1 | 22.18 ± 0.39 | 1.6 ± 0.3 | – | 30.44 | 30.73 | 30.81 | 30.91 | 31.35 | |||
| 349 | yes/III | 061325.94+175923.5 F | 95.6 | 20.0∗ | 1.0 ± 0.3 | – | 30.48 | 29.73 | 29.73 | 30.55 | 30.56 | |||
| 354 | yes | 061327.41+175554.3 | 125.2 | 21.91 ± 0.3 | 5.6 ± 4.1 | – | 30.25 | 30.82 | 30.85 | 30.93 | 31.08 | |||
| 355 | yes | 061327.61+175517.8 | 182.8 | 22.11 ± 0.35 | 3.8 ± 1.4 | – | 30.38 | 31.00 | 31.05 | 31.10 | 31.32 | |||
| 359 | yes | 061328.37+175604.4 | 97.7 | 22.15 ± 0.52 | 4.3 ± 2.6 | – | 30.07 | 30.75 | 30.80 | 30.84 | 31.06 | |||
Notes. The spectral fit was performed with an absorbed thermal plasma model with one (tbabs*vapec) or two components (tbabs*(vapec+vapec)). ∗ Indicates frozen parameters in the fit. Column (2): presence of an optical or infrared counterpart, infrared class from Spitzer photometry (if available). Column (3): sources flagged with “F” showed flare-like variability during our observations; lightcurves are shown in Fig. 6; Col. (4): absorbing hydrogen column density of the best-fit; Cols. (5) and (6): plasma temperature(s) of the best-fit; Cols. (7) to (11): X-ray luminosities (for an assumed distance of 1.6 kpc) in the soft (s, [0.5−2.0] keV) band, the hard (h, [2.0−8.0] keV) band, and the total (t, [0.5−8.0] keV) band. Absorption-corrected luminosities are denoted with the subscript c.
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