Table 1.
Properties of the galaxies in the sample
| Source | z | WISE | LFIR | v50 | v84 | EWabs | EW |
Fluxabs | Ṁmol |
|---|---|---|---|---|---|---|---|---|---|
| class. | (1012 L⊙) | (km s−1) | (km s−1) | (km s−1) | (km s−1) | (Jy km s−1) | (M⊙ yr−1) | ||
| IRAS F13352+6402 | 0.2360 (a) | Sy/QSO | 2.9 (d) | −115 | −480 | 338 | 115 | 182 ± 9 | ∼570 (g) |
| IRAS F10091+4704 | 0.2451 (b) | SB | 3.7 (d) | +430 | +75 | 211 | − | 112 ± 7 | ∼100 (h) |
| IRAS F20036−1547 | 0.1920 (a) | Sy/QSO | 2.9 (d) | −70 | −455 | 184 | 58 | 170 ± 9 | ∼290 (g) |
| IRAS F18216+6419 | 0.2974 (a) | Sy/QSO | 6.9 (d) | − | − | − | − | < 18 (f) | − |
| J131911+095051 | 6.1330 (c) | QSO | 25.1 (e) | −154 | −314 | 38.4 | 14.4 | 0.14±0.048 | ∼200 (g) |
Notes.
Redshift from Wang & Rowan-Robinson (2009).
Redshift from Rupke et al. (2005).
Redshift from Wang et al. (2013).
LFIR from Wang & Rowan-Robinson (2009).
Calculated from the modeling of the spectral energy distribution (see Appendix B).
Calculated using Eq. (C.1).
This value corresponds to an inflow rate (see Sect. 4.2).
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