Sample of local ULIRGs.
|(ICRS)||(ICRS)||(km s−1)||(Mpc)||(pc arcsec−1)|
Notes. (a) Coordinates of the 248 GHz rest-frame continuum emission for each nucleus (see Sect. 3.1.2). The astrometric uncertainty is ~25 mas (see Sect. 3.2). (b) CO(2–1) systemic velocity using the relativistic velocity definition in the kinematic local standard of rest (LSRK; see Sect. 3.2). Typical uncertainties are ≲10 km s−1. (c) Redshift using the average systemic velocity of the system. (d)Luminosity distance and scale for the assumed cosmology (see Sect. 1). (e) Luminosity of the AGNin the system estimated from mid-IR spectroscopy (Veilleux et al. 2009). (f) IR luminosity of the system based on the SED fitting of the Spitzer and Herschel mid- and far-IR photometry (see Sect. 3.4.1). (*)No 248 GHz continuum is detected at the position of the near-IR W nucleus of IRAS 22491−1808.
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