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Table 1

The SINFONI sample.

ID1 ID2 z DL Scale log (LIR/L)
Common IRAS (Mpc) (pc/")
(1) (2) (3) (4) (5) (6)

IRAS 06206-6315 IRAS 06206-6315 0.092441 425 1726 12.31
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
IRAS 12112+0305 IRAS 12112+0305 0.073317 337 1416 12.38
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
IRAS 14348-1447 IRAS 14348-1447 0.083000 382 1575 12.41
IRASF 17138-1017 IRAS 17138-1017 0.017335 75.3 353 11.42
IRAS 17208-0014 IRAS 17208-0014 0.042810 189 844 12.43
IC 4687 IRAS 18093-5744 0.017345 75.1 352 11.44
IRAS 21130-4446 IRAS 21130-4446 0.092554 421 1712 12.22
NGC 7130 IRAS 21453-3511 0.016151 66.3 312 11.34
IC 5179 IRAS 22132-3705 0.011415 45.6 216 11.12
IRAS 22491-1808 IRAS 22491-1808 0.077760 347 1453 12.23
IRAS 23128-5919 IRAS 23128-5919 0.044601 195 869 12.04

Notes. Column (3): redshift from the NASA Extragalactic Database (NED). Columns (4) and (5): Luminosity distance and scale from Ned Wright’s Cosmology Calculator (Wright 2006) given h0 = 0.70, ΩM = 0.7, ΩM = 0.3. Column (6): LIR (8–1000μm) 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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