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Table 5

Results from the SED fits for the X-ray detected DOGs.

LID z log LIR(8−1000 μm) log L12 μm log stellar mass SFR
L erg s-1 erg s-1 erg s-1 erg s-1 M M/yr
(1) (2) (3) (4) (5) (6) (7) (8) (9)

95 5.22 13.45 46.28 46.08 45.85 43.93 12.30 4029
117 1.51 11.47 44.38 44.04 44.12 41.96 9.87 37
170 1.22 11.51 44.09 44.08 42.16 41.96 10.91 56
197 1.81 12.11 44.82 44.82 42.59 42.42 11.11 220
199 2.45 12.38 45.09 45.08 41.97 42.75 11.34 410
230 2.61 12.50 44.96 44.87 44.23 42.82 11.51 525
232 2.291 12.39 45.34 44.91 45.13 42.85 10.76 272
293 3.88 13.55 46.26 46.26 42.74 42.30 10.95 6164
307 1.90 11.71 44.50 44.36 43.93 41.87 10.52 79
309 2.579 13.01 45.74 45.71 44.59 42.82 11.33 1722
321 1.603 12.22 45.33 44.34 45.28 42.69 10.93 75
326 3.10 12.66 45.37 45.37 42.70 11.35 790
346 1.221 11.87 44.78 44.41 44.54 41.49 9.21 90
397 2.28 11.94 44.65 44.65 42.65 11.17 150

Notes. The columns are: (1) Chandra ID from the Luo et al. (2010) catalogue. (2) Redshift. (3) Total IR luminosity (8–1000 μm). (4) Total luminosiy at 12 μm. (5) Luminosity of the starburst component at 12 μm. (6) Luminosity of the AGN component at 12 μm. (7) Luminosity of the stellar component at 12 μm. (8) Stellar mass. (9) Star formation rate.

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