Table 4.
Best-fit parameters of the SED decomposition.
| XID | M* | LIR | Lbol | E(B−V) | fAGN | SFR | Mgas |
|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| 42 | 2.16 ± 0.65 | 9.62 ± 1.92 | 2.60 ± 0.78 | 0.31 | 0.01 | 1679 ± 336 | 5.41 ± 3.21 |
| 170 | 1.74 ± 0.52 | 1.57 ± 0.31 | 1.89 ± 0.57 | 0.24 | 0.02 | 276 ± 55 | 0.87 ± 0.51 |
| 337 | 3.43 ± 1.03 | 1.01 ± 0.20 | 3.11 ± 0.93 | 0.24 | 0.09 | 192 ± 38 | 0.85 ± 0.51 |
| 539 | 2.15 ± 0.64 | 4.90 ± 0.98 | 2.66 ± 0.80 | 0.37 | 0.02 | 864 ± 173 | 4.55 ± 2.70 |
| 551 | 2.19 ± 0.66 | 2.27 ± 0.45 | 2.92 ± 0.88 | 0.36 | 0.14 | 456 ± 91 | 0.88 ± 0.52 |
| 666 | 4.41 ± 1.32 | 4.90 ± 0.98 | 4.82 ± 1.44 | 0.38 | 0.03 | 872 ± 175 | 2.76 ± 1.63 |
| 746 | 4.33 ± 1.30 | 1.44 ± 0.29 | 2.84 ± 0.85 | 0.48 | 0.17 | 299 ± 60 | 0.80 ± 0.47 |
Notes. (1) X-ray source ID (see Table 1); (2) stellar mass in units of 1011 M⊙; (3) total infrared luminosity integrated in the rest-frame 8−1000 μm range in units of 1012 L⊙; (4) AGN bolometric luminosity in units of 1012 L⊙; (5) attenuation to the stellar emission; (6) fractional AGN contribution to the total IR luminosity; (7) SFR in units of M⊙ yr−1; and (8) Mgas = MH2 + MHI in units of 1010 M⊙. Errors are given at the 68% confidence level. Relative errors are ∼30% for stellar masses and ∼20% for IR luminosities and AGN bolometric luminosities.
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