Fig. 6.
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Rest-frame 6 μm AGN luminosity (L6 μm) as a function of redshift. The L6 μm is estimated from the decomposed AGN dust component as a result of the SED fitting, as discussed in Section 2.4. The red stars denote the eFEDS-DOGs, and the blue squares denote eFEDS-DOGs with the BluDOG-like feature. The lime, magenta, cyan, and pink plots represent X-ray detected DOGs from Lanzuisi et al. (2009), Toba et al. (2020), Zou et al. (2020), and Kayal & Singh (2024), respectively. As for the hot DOG samples, black triangle, downward triangle, pentagon, square, and cross represent data from Stern et al. (2014), Assef et al. (2016), Zappacosta et al. (2018), Ricci et al. (2017a) and Vito et al. (2018), respectively.
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