AGN host stellar mass vs. absolute K_s-band magnitude using the KEx (left panel) and the MEx (right panel) line diagnostic methods. The horizontal dashed line shows the stellar mass completeness obtained by Laigle et al. (2016) for the regions called 𝒜^Deep (dotted lines) and 𝒜^UD in the redshift range 0.35 < z < 0.65 and 0.65 < z < 0.95, respectively. The upper and right panels in each figure show the absolute K_s band and the stellar mass distributions for each sample. Circles, squares, crosses, and triangles represent pre-selected AGNs according to the methods of S05, L04, Ch17, and M12, respectively.