Table 1
LIRG sample.
| ID1 | ID2 | z | DL | Scale | log (LIR/L⊙) |
| common | IRAS | (Mpc) | (pc/′′) | ||
| (1) | (2) | (3) | (4) | (5) | (6) |
|
|
|||||
| NGC 2369 | IRAS 07160-6215 | 0.010807 | 48.6 | 230 | 11.17 |
| NGC 3110 | IRAS 10015-0614 | 0.016858 | 78.4 | 367 | 11.34 |
| NGC 3256 | IRAS 10257-4338 | 0.009354 | 44.6 | 212 | 11.74 |
| ESO 320-G030 | IRAS 11506-3851 | 0.010781 | 51.1 | 242 | 11.35 |
| IRASF 12115-4656 | IRAS 12115-4657 | 0.018489 | 84.4 | 394 | 11.10 |
| NGC 5135 | IRAS 13229-2934 | 0.013693 | 63.5 | 299 | 11.33 |
| IRASF 17138-1017 | IRAS 17138-1017 | 0.017335 | 75.3 | 353 | 11.42 |
| IC 4687 | IRAS 18093-5744 | 0.017345 | 75.1 | 352 | 11.44 |
| NGC 7130 | IRAS 21453-3511 | 0.016151 | 66.3 | 312 | 11.34 |
| IC 5179 | IRAS 22132-3705 | 0.011415 | 45.6 | 216 | 11.12 |
Notes. Column (3): redshift from the NASA Extragalactic Database (NED). Columns (4) and (5): luminosity distance and scale derived using Ned Wright’s Cosmology Calculator (Wright 2006) given h0 = 0.70, ΩM = 0.7, ΩM = 0.3. Column (6): LIR(8–1000 μm) calculated from the IRAS flux densities f12, f25, f60 and f100 (Sanders et al. 2003), using the expression given in Sanders & Mirabel (1996). A complete version of this table can be found in Piqueras López et al. (2012).
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