Table A.1.
Sample of U/LIRGs used for the analysis.
| RBGS Name | AllWISE name | RA | Dec | Distance | LIR |
|---|---|---|---|---|---|
| deg | deg | Mpc | log(L⊙) | ||
| NGC 0023 | J000953.41+255526.0 | 2.4726 | 25.9239 | 64.4 | 11.12 |
| NGC 0034 | J001106.54−120627.5 | 2.7773 | −12.1076 | 82.8 | 11.50 |
| MCG-02-01-051/2 | J001850.89−102236.8 | 4.7121 | −10.3769 | 115.0 | 11.48 |
| MCG-02-01-051/2 | J001849.98−102140.1 | 4.7083 | −10.3612 | 115.0 | 11.48 |
| ESO 350-IG038 | J003652.45−333316.9 | 9.2186 | −33.5547 | 87.6 | 11.29 |
| NGC 0232 | J004245.81−233341.0 | 10.6909 | −23.5614 | 95.5 | 11.46 |
| ... |
The RBGS name for a galaxy being the same in multiple rows indicates that multiple WISE sources are associated with that galaxy, and the AllWISE names can be used to identify these sources. As described in the text, the distances are obtained from the NED and the value of LIR is updated from that given in the RBGS. The full table is available at the CDS.
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