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The host galaxies of X ray selected active galactic nuclei to z = 2 5 : structure, star formation, and their relationships from CANDELS and Herschel/PACS

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Figure

Fig. 1. The breakup of the mean scatter of visual classification metrics for galaxies at 0The mean scatter for a galaxy is defined as the average absolute value of the di.5 < z < 2.5 binned by their final mean metric value.fference of the metric between pairs
Fig. 2. A montage of randomly chosen inactive galaxies at 1row of five galaxies are randomly selected from all objects in one of the three bins in IM (see Sect.each panel and IM is written at the lower left
Table 1. Total AGN/inactive sample sizes after the application of different selections.
Fig. 4. Top panels: physical half-light semi-major axis radii plotted against stellar mass M∗ for AGNs (large red points), inactive control galaxies(large black points) and the overall galaxy population (small grey points), in four distinct redshift bins
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