Fig. 1.
Distributions of the basic properties of our galaxy sample. The redshift distribution is plotted in the top-left panel and the number of sources per merging class is in the top-right panel. In the bottom-left panel, the IR luminosity distribution, based on IRAS observations (Sanders et al. 2003) is shown, while the bolometric AGN fractions calculated in Díaz-Santos et al. (2017) are plotted in the bottom-right panel.
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