Fig. 2
Emission-line FWHM (top) and velocity offset (bottom) as a function of stellar mass, as estimated by Seymour et al. (2007) and De Breuck et al. (2010) from Spitzer near- to mid-infrared photometry. The red dots show the galaxies from our sample, the small black empty squares the stellar-mass selected sample of Buitrago et al. (2014) without powerful AGN for comparison. We do not find a correlation for our sample in either relationship.
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