Table 1
Photometry.
| ID | α | δ | f 0.5−10 keV | R | f 3.6 μm | f 24 μm | f 850 μm | LR | z | Ref. |
| (1) | (2) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
|
|
||||||||||
| W-4 | 52.8996 | –27.9121 | 1.85 | 24.94 | 7.00 ± 0.10 | 139 ± 5 | 11.0 ± 1.2 | 5.00 | 2.58 ± 0.9 | 1 |
| W-9 | 53.0475 | –27.8704 | 7.14 | 26.02 | 9.83 ± 0.05 | 122 ± 5b | 9.4 ± 1.2 | 6.92 | 3.99 ± 0.08 | 2 |
| W-11 | 53.0577 | –27.9334 | 1.33 | 25.61 | 6.83 ± 0.07 | 113 ± 6 | 9.2 ± 1.2 | 5.06 | 6.07 ± 1.1 | 2 |
| W-40 | 53.1950 | –27.8557 | 0.44 | 24.35 | 8.51 ± 0.15 | 140 ± 4b | 6.4 ± 1.2 | 6.08 | 1.90 ± 0.02 | 2 |
| W-45 | 53.1052 | –27.8752 | 0.06 | 27.41 | 7.50 ± 0.27 | 141 ± 4 | 6.3 ± 1.2 | 1.50 | 2.50 ± 0.2 | 2 |
| W-57 | 52.9665 | –27.8908 | 1.51 | 24.33 | 7.60 ± 0.10 | 273 ± 6 | 6.1 ± 1.3 | 12.81 | 2.940 | 3 |
| W-59 | 53.2658 | –27.7362 | 1.35 | 25.62 | 30.28 ± 0.10a | 453 ± 5a | 6.0 ± 1.3 | 7.67 | 1.38 ± 0.02 | 2 |
| W-66 | 53.3830 | –27.9028 | 36.1 | 20.72 | 56.34 ± 0.13 | 679 ± 9.4 | 6.1 ± 1.3 | 5.37 | 0.58 ± 0.03 | 5 |
| W-67 | 53.1803 | –27.9206 | 0.29 | 24.20 | 21.7 ± 0.9 | 554 ± 4a | 5.9 ± 1.3 | 15.77 | 2.122 | 4 |
| W-84 | 52.9773 | –27.8513 | 1.58 | 24.97 | 12.98 ± 0.09 | 231 ± 4b | 5.5 ± 1.3 | 4.16 | 3.2 ± 0.06 | 2 |
| W-92 | 52.9096 | –27.7277 | 2.98 | 24.49 | 26.57 ± 0.10 | 80 ± 5 | 5.2 ± 1.2 | 2.69 | 2.10 ± 0.04 | 5 |
| W-101 | 52.9643 | –27.7649 | 1.16 | 23.01 | 5.33 ± 0.10 | 34 ± 2.9 | 5.1 ± 1.3 | 0.66 | 2.53 ± 0.12 | 2 |
| W-108 | 53.3175 | –27.8445 | 1.75 | 17.36 | 516.74 ± 0.10 | 4040 ± 100c | 5.0 ± 1.2 | 7.89 | 0.0875 | 6 |
| W-114 | 52.9628 | –27.7436 | 3.11 | 23.88 | 51.63 ± 0.10 | 660 ± 9 | 4.9 ± 1.3 | 2.85 | 1.605 | 7 |
Notes. The columns are: (1) LABOCA source number in Weiß et al. (2009); (2) X-ray counterpart equatorial coordinates; (3) Total band X-ray flux in units of × 10-15 erg s-1 cm-2; (4) R-band magnitude (AB); (5) 3.6 μm flux in units of μJy; (6) 24 μm flux in units of μJy. (9) Redshift: Three and two decimal digits denote a spectroscopic and a photometric redshift respectively (10).
Lower limit (7) LABOCA 870 μm flux in units of mJy. (8) Likelihood-ratio between LABOCA and MIPS counterpart.
References. 1) EAZY; 2) Luo et al. (2010); 3) Szokoly et al. (2004); 4) Kriek et al. (2006); 5) Taylor et al. (2009); 6) Norris et al. (2006); 7) Chapin et al. (2010).
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