Table 1.
Sample galaxies.
| Name | RA | Dec | z | DL(a) | LFIR(b) | LIR(c) | f25/f60(d) | Incl. (e) |
|---|---|---|---|---|---|---|---|---|
| (J2000) | (J2000) | (Mpc) | (1011 L⊙) | (1011 L⊙) | (°) | |||
| ULIRGs | ||||||||
| IRAS 17208–0014 | 17:23:21.95 | −00:17:00.9 | 0.0428 | 183 ± 12 | 22 | 25 ± 3 | 0.05 | 90 |
| IRAS F14348–1447 | 14:37:38.32 | −15:00:24.0 | 0.0830 | 362 ± 24 | 18 | 20 ± 3 | 0.08 | 69 |
| IRAS F12112+0305 | 12:13:46.08 | +02:48:41.5 | 0.0733 | 318 ± 21 | 17 | 19 ± 3 | 0.08 | 22 |
| IRAS 13120–5453 | 13:15:06.33 | −55:09:22.8 | 0.0311 | 135 ± 9 | 15 | 18 ± 2 | 0.07 | 41 |
| IRAS 09022–3615 | 09:04:12.72 | −36:27:01.3 | 0.0596 | 253 ± 17 | 15 | 18 ± 2 | 0.10 | 37 |
| Arp 220 | 15:34:57.27 | +23:30:10.5 | 0.0181 | 81.8 ± 5.5 | 14 | 16 ± 2 | 0.08 | 57 |
| IRAS F14378–3651 | 14:40:59.01 | −37:04:31.9 | 0.0682 | 295 ± 20 | 12 | 14 ± 2 | 0.10 | … |
| IRAS F22491–1808 | 22:51:49.31 | −17:52:24.0 | 0.0778 | 328 ± 22 | 12 | 13 ± 2 | 0.10 | … |
| LIRGs | ||||||||
| NGC 1614 | 04:34:00.03 | −08:34:44.6 | 0.0159 | 64.1 ± 4.3 | 2.7 | 4.0 ± 0.5 | 0.23 | 42 |
| NGC 7469 | 23:03:15.67 | +08:52:25.3 | 0.0164 | 66.5 ± 4.4 | 2.5 | 3.9 ± 0.5 | 0.22 | 30 |
| NGC 3256 | 10:27:51.23 | −43:54:16.6 | 0.0094 | 36.1 ± 2.4 | 2.7 | 3.7 ± 0.5 | 0.15 | 48 |
| IRAS F17138–1017 | 17:16:35.70 | −10:20:38.0 | 0.0173 | 77.3 ± 5.2 | 1.8 | 2.6 ± 0.3 | 0.14 | 71 |
| IRAS 17578–0400 | 18:00:31.85 | −04:00:53.5 | 0.0134 | 60.0 ± 4.1 | 2.0 | 2.3 ± 0.3 | 0.04 | 81 |
| NGC 7130 | 21:48:19.52 | −34:57:04.8 | 0.0163 | 68.1 ± 4.6 | 1.7 | 2.3 ± 0.3 | 0.13 | 34 |
| ESO 173–G015 | 13:27:23.77 | −57:29:22.1 | 0.0100 | 32.7 ± 2.3 | 1.8 | 2.2 ± 0.3 | 0.09 | 90 |
| NGC 3110 | 10:04:02.12 | −06:28:29.1 | 0.0169 | 74.3 ± 5.0 | 1.6 | 2.0 ± 0.3 | 0.10 | 65 |
| IC 4734 | 18:38:25.69 | −57:29:25.8 | 0.0156 | 67.8 ± 4.5 | 1.7 | 1.9 ± 0.3 | 0.09 | 57 |
| Zw 049.057 | 15:13:13.10 | +07:13:32.0 | 0.0130 | 60.2 ± 4.1 | 1.7 | 1.9 ± 0.3 | 0.04 | 44 |
| NGC 5135 | 13:25:44.06 | −29:50:01.2 | 0.0137 | 52.6 ± 3.5 | 1.1 | 1.5 ± 0.2 | 0.14 | 25 |
| ESO 221–IG10 | 13:50:56.92 | −49:03:19.7 | 0.0105 | 59.0 ± 11.0 | 1.0 | 1.5 ± 0.6 | 0.14 | 24 |
| IC 5179 | 22:16:09.09 | −36:50:37.5 | 0.0113 | 47.3 ± 3.2 | 1.1 | 1.5 ± 0.2 | 0.12 | 62 |
| UGC 2982 | 04:12:22.67 | +05:32:49.1 | 0.0177 | 70.6 ± 4.7 | 1.0 | 1.4 ± 0.2 | 0.10 | 64 |
| ESO 286-G035 | 21:04:11.16 | −43:35:32.5 | 0.0174 | 73.2 ± 4.9 | 1.0 | 1.3 ± 0.2 | 0.09 | 79 |
| NGC 4418 | 12:26:54.62 | −00:52:39.4 | 0.0073 | 33.2 ± 2.2 | 1.0 | 1.3 ± 0.2 | 0.22 | 68 |
| NGC 2369 | 07:16:37.75 | −62:20:37.5 | 0.0108 | 44.6 ± 3.0 | 1.0 | 1.3 ± 0.2 | 0.11 | 90 |
| NGC 5734 | 14:45:09.05 | −20:52:13.8 | 0.0136 | 60.2 ± 4.0 | 1.0 | 1.1 ± 0.2 | 0.09 | 58 |
| ESO 320–G030 | 11:53:11.72 | −39:07:49.1 | 0.0103 | 36.0 ± 2.5 | 1.0 | 1.1 ± 0.2 | 0.07 | 64 |
| sub-LIRGs | ||||||||
| NGC 1068(f) | 02:42:40.77 | −00:00:47.8 | 0.0038 | 15.8 ± 1.1 | 0.78 | 2.5 ± 0.3 | 0.45 | 35 |
| NGC 1808 | 05:07:42.34 | −37:30:47.0 | 0.0034 | 13.1 ± 0.9 | 0.35 | 0.56 ± 0.08 | 0.16 | 83 |
| NGC 4254 | 12:18:49.63 | +14:24:59.4 | 0.0080 | 15.3 ± 2.8 | 0.26 | 0.34 ± 0.10 | 0.12 | 20 |
| NGC 4303 | 12:21:54.95 | +04:28:24.9 | 0.0052 | 15.3 ± 2.8 | 0.23 | 0.32 ± 0.10 | 0.13 | 18 |
| NGC 660 | 01:43:02.35 | +13:38:44.5 | 0.0028 | 12.3 ± 0.8 | 0.24 | 0.31 ± 0.04 | 0.11 | 79 |
| NGC 4527 | 12:34:08.50 | +02:39:13.7 | 0.0058 | 15.3 ± 2.8 | 0.19 | 0.26 ± 0.10 | 0.11 | 81 |
| NGC 3627 | 11:20:15.03 | +12:59:28.6 | 0.0024 | 10.0 ± 1.1 | 0.17 | 0.24 ± 0.05 | 0.13 | 68 |
| NGC 613 | 01:34:18.24 | −29:25:06.6 | 0.0049 | 15.0 ± 3.0 | 0.17 | 0.23 ± 0.09 | 0.16 | 36 |
| NGC 4666 | 12:45:08.68 | −00:27:42.9 | 0.0051 | 12.8 ± 2.6 | 0.17 | 0.23 ± 0.09 | 0.10 | 70 |
| NGC 1792 | 05:05:14.45 | −37:58:50.7 | 0.0040 | 12.5 ± 2.5 | 0.17 | 0.21 ± 0.09 | 0.12 | 63 |
| NGC 4501 | 12:31:59.22 | +14:25:13.5 | 0.0076 | 15.3 ± 2.8 | 0.17 | 0.21 ± 0.08 | 0.15 | 63 |
| NGC 4536 | 12:34:27.13 | +02:11:16.4 | 0.0060 | 14.9 ± 3.0 | 0.15 | 0.21 ± 0.08 | 0.13 | 73 |
| NGC 5643 | 14:32:40.78 | −44:10:28.6 | 0.0040 | 14.4 ± 1.0 | 0.12 | 0.19 ± 0.03 | 0.20 | 30 |
| NGC 3628 | 11:20:17.02 | +13:35:22.2 | 0.0028 | 10.0 ± 1.1 | 0.14 | 0.17 ± 0.04 | 0.09 | 79 |
| NGC 1559 | 04:17:35.78 | −62:47:01.3 | 0.0043 | 12.7 ± 2.5 | 0.13 | 0.16 ± 0.07 | 0.10 | 60 |
| NGC 5248 | 13:37:32.07 | +08:53:06.2 | 0.0038 | 13.8 ± 2.8 | 0.12 | 0.16 ± 0.06 | 0.14 | 56 |
| NGC 3810 | 11:40:58.74 | +11:28:16.1 | 0.0033 | 15.4 ± 3.1 | 0.10 | 0.13 ± 0.05 | 0.12 | 48 |
| NGC 4654 | 12:43:56.64 | +13:07:34.9 | 0.0035 | 15.3 ± 2.8 | 0.10 | 0.12 ± 0.05 | 0.13 | 60 |
| NGC 1055 | 02:41:45.18 | +00:26:38.1 | 0.0033 | 11.3 ± 2.3 | 0.10 | 0.12 ± 0.05 | 0.12 | 63 |
Notes.
Luminosity distances calculated from the redshifts following the procedure outlined by Sanders et al. (2003). For consistency, in galaxies where Sanders et al. (2003) instead use direct primary or secondary distance measurements, we use the same distances as they do. For the same reason, a H0 = 75 km s−1 Mpc−1, Ωm = 0.3, and ΩΛ = 0.7 cosmology is adopted.
Far-infrared luminosities used for selection, taken from Sanders et al. (2003).
Infrared luminosities calculated using the prescription in Table 1 of Sanders & Mirabel (1996, originally from Pérault 1987) using IRAS fluxes taken from Sanders et al. (2003).
Ratio of IRAS fluxes at 25 μm and 60 μm taken from Sanders et al. (2003).
Inclinations of the host galaxies taken from the HyperLEDA database (http://leda.univ-lyon1.fr/) (Makarov et al. 2014).
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