Number of galaxies and total IR luminosity range of the local galaxy samples.
|samples||Nb||R radio||FEE||<10||10–11||11–12||≥ 12|
Notes. Column (2) total number of objects for each local sample; Col. (3) number of galaxies with a radio continuum (1.4 GHz) size estimate; Col. (4) number of galaxies for which a fraction of extended emission (FEE) was measured (Díaz-Santos et al. 2010), i.e., fraction of the mid-IR continuum at 13.2 μm more extended than the Spitzer/IRS resolution of 3.6″ (see Sect. 5).
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