Table 1.
Galaxies analyzed in this work along with some general properties.
| Galaxy name | z | DL | RA | Dec | αAGN | log LIR | log LAGN | SFR | Ref. |
|---|---|---|---|---|---|---|---|---|---|
| [Mpc] | [L⊙] | [L⊙] | [M⊙ yr−1] | ||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
| IRAS F01572+0009 | 0.1631 | 806.66 | 01:59:50.253 | +00:23:40.87 | 0.65 | 12.62 | 12.49 | 150 ± 60 | β |
| IRAS 03521+0028 | 0.1519 | 746.13 | 03:54:42.219 | +00:37:03.41 | 0.06 | 12.52 | 11.39 | 309 ± 120 | γ |
| IRAS F05189−2524 | 0.0426 | 194.52 | 05:21:01.392 | −25:21:45.36 | 0.72 | 12.16 | 12.07 | 40 ± 16 | β |
| IRAS 06035−7102 | 0.0795 | 372.55 | 06:02:54.066 | −71:03:10.48 | 0.60 | 12.22 | 12.06 | 70 ± 30 | γ |
| IRAS 06206−6315 | 0.0924 | 436.81 | 06:21:01.210 | −63:17:23.5 | 0.43 | 12.23 | 11.92 | 100 ± 40 | γ |
| IRAS 08311−2459 | 0.1005 | 477.67 | 08:33:20.600 | −25:09:33.7 | 0.79 | 12.50 | 12.46 | 70 ± 30 | γ |
| IRAS 09022−3615 | 0.0596 | 275.47 | 09:04:12.689 | −36:27:00.76 | 0.55 | 12.29 | 12.09 | 90 ± 30 | β |
| IRAS 10378+1109 | 0.1363 | 663.02 | 10:40:29.169 | +10:53:18.29 | 0.30 | 12.31 | 11.85 | 140 ± 60 | γ |
| IRAS F12112+0305 | 0.07309 | 341.01 | 12:13:45.978 | +02:48:40.4 | 0.18 | 12.32 | 11.63 | 170 ± 70 | β |
| IRAS F13451+1232 | 0.1217 | 586.51 | 13:47:33.425 | +12:17:24.32 | 0.81 | 12.32 | 12.29 | 41 ± 15 | β |
| IRAS 16090−0139 | 0.1336 | 648.77 | 16:11:40.432 | −01:47:06.56 | 0.43 | 12.55 | 12.25 | 200 ± 80 | γ |
| IRAS 17208−0014 | 0.0428 | 195.47 | 17:23:21.920 | −00:17:00.7 | ≤0.05 | 12.39 | 11.15 | 230 ± 90 | β |
| IRAS 19254−7245 | 0.06149 | 284.58 | 19:31:21.400 | −72:39:18.0 | 0.74 | 12.09 | 12.02 | 32 ± 12 | γ |
| IRAS F20551−4250 | 0.0430 | 196.41 | 20:58:26.781 | −42:39:00.20 | 0.57 | 12.05 | 11.87 | 48 ± 19 | β |
| IRAS F22491−1808 | 0.0778 | 364.16 | 22:51:49.264 | −17:52:23.46 | 0.14 | 12.84 | 12.05 | 590 ± 220 | β |
| IRAS F23060+0505 | 0.1730 | 860.75 | 23:08:33.952 | +05:21:29.76 | 0.78 | 12.53 | … | 80 ± 30 | δ |
| IRAS F23128−5919 | 0.0446 | 203.95 | 23:15:46.749 | −59:03:15.55 | 0.63 | 12.03 | 11.89 | 40 ± 15 | β |
Notes. (1) Source name. (2) Redshift. (3) Luminosity distance. (4) Right ascension. (5) Declination. (6) Reported fractional contribution of the AGN to the bolometric luminosity in the reference papers (αAGN = LAGN/Lbol). (7) Infrared luminosity (8 − 1000 μm). (8) AGN luminosity. (9) Star formation rate.
References. β: Veilleux et al. (2013), γ: Spoon et al. (2013), δ: Fluetsch et al. (2019).
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