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Table 3.

IR properties of OHM candidates.

AGC name WISE coords WISE[3.4] WISE[4.6] WISE[12] WISE[22] F60 F100 LFIR
(mag) (mag) (mag) (mag) (Jy) (Jy) (log L)
102708 J000336.00+253202.7 17.78 16.40 12.65 9.06 0.015 0.048 10.35
102850 J002958.27+305833.9 14.24 14.01 10.17 8.08 0.018 0.034 10.34
114732 J010107.16+094624.3 16.61 16.12 11.83 8.69 0.019 0.054 10.43
115713 J014135.21+165730.6 14.73 14.04 9.64 6.90 0.109 0.308 11.19
115018 J015847.20+073202.6 16.60 16.71 12.64 8.79 0.012 0.035 10.41
124351 J021750.86+072428.7 16.84 16.48 12.73 9.26 0.007 0.019 10.0
749309SE J101103.18+273925.7 17.25 16.58 11.84 9.06 0.019 0.060 10.58
749309NW J101100.37+274036.6 14.39 14.10 12.02 8.73 0.003 0.005 9.63
219835 J113033.78+322139.3 14.89 14.50 11.97 8.70 0.005 0.009 9.91
249507 J140340.36+295456.6 14.84 14.24 10.33 7.85 0.29* 0.70* 11.63*
322231 J223605.38+095726.2 14.66 14.35 12.38 8.71 0.004 0.006 9.62

Notes. Columns 2–6: WISE coordinate and four-band data. Columns 7–8: FIR flux at 60 and 100 μm band. The “*” symbol stands for the IR flux from the IRAS survey, others are derived from WISE data from Columns 3–6. Column 9: Integrated FIR luminosity using the method from Baan & Klöckner (2006; see text for details). We used the same redshift for calculating the luminosity, as given in Table 1.

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