Table 5
Infrared properties of heavily obscured sources.
| PID | z | L 12 | L 8 − 1000 | AGN frac. | log M⋆ | SFR | sSFR |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
|
|
|||||||
| 48 | 0.297 | 1.66 | 1.05 | 0.25 | 10.51 | 1.26 | –0.48 |
| 66 | 1.185 | 4.21 | 1.40 | 0.22 | 11.21 | 1.39 | –1.05 |
| 144 | 3.700 | 14.60 | 33.7 | 0.01 | 10.87 | 2.77 | 0.67 |
| 147 | 1.530 | 7.37 | 3.33 | 0.10 | 10.81 | 1.76 | –0.28 |
| 214 | 2.00 | 9.5 | 6.5 | 0.95 | 10.52 | 1.90 | –0.99 |
| 222 | 0.424 | 0.11 | –† | – | 10.64 | – | – |
| 245 | 2.68 | 17.7 | 6.6 | 0.05 | 10.34 | 2.05 | 0.56 |
| 289 | 0.605 | 1.25 | 2.0 | 0.22 | 10.81 | 1.43 | –0.61 |
| 324 | 1.222 | 75.3 | 8.3 | 0.36 | 10.84 | 1.96 | –0.11 |
Notes.The columns are: (1) XMM-ID; (2) redshift; (3) rest-frame 12 μm luminosity in units of solar luminosities (× 1010); (4) total IR luminosity in units of solar luminosities (× 1011); (5) AGN fraction of the total IR luminosity; (6) logarithm of stellar mass in units of solar masses; (7) logarithm of star-formation rate in units of solar masses/yr; (8) specific star-formation rate in units of Gyr-1.
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