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Table 1
Sample galaxies.
| Name | RA | Dec | Log LFIR | D | Type | Telescope | Beam | Sensitivity⋆ |
| (J2000) | (J2000) | [L⊙] | [Mpc] | ( ) |
(mJy/channel) | |||
|
|
||||||||
| IC 860 | 13:15:03.05 | +24:37:08.0 | 11.17 | 59 | Sab | IRAM PdBI |
|
1.2 mJy |
| Zw049.057 | 15:13:13.10 | +07:13:32.0 | 11.27 | 59 | Sab | IRAM PdBI |
|
1.6 mJy |
| Arp220W | 15:34:57.27 | +23:30:10.5 | 12.03 | 80 | merger | ALMA |
|
1.9 mJy |
| IRAS 17208−0014 | 17:23:21.94 | −00:17:01.0 | 12.39 | 176 | merger | ALMA |
|
1.6 mJy |
Notes. LIR and D from Sanders et al. (2003) (where D is the angular distance (DA)) but for Arp220W we attempt to estimate the luminosity emerging from the western nucleus only from the continuum study of Sakamoto et al. (2008).
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