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Fig. 6.

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WISE diagram as a function of the AGN fraction for DESI galaxies observed with S/N ≥ 3 at W1 − 3 (left panel) or at all WISE bands (i.e., FLAGINFRARED = 4; right panel). The region of AGNs is marked by a dotted red line and follows the criterion proposed by Hviding et al. (2022). The WISE-selected AGNs are characterized by a higher AGN fraction than non-AGN galaxies except for the SED-MIR-AGN candidates, which are characterized by a high AGN fraction (AGNFRAC ≳ 0.5 at the right panel). We note that 96% of these SED-MIR-AGNs missed by the WISE diagram are identified as AGNs by the TBT diagram.

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