Luminosities of eFEDS-WERGS sample as a function of redshift. The points are the same as in Fig. 1. Top: rest-frame radio luminosity log L_1.4 GHz (W Hz⁻¹) as a function of redshift, where L_1.4 GHz is obtained from VLA/FIRST (Helfand et al. 2015), and the k-correction was made by Yamashita et al. (2018) based on redshift. The green stars and orange circle and red star points are data obtained from the FIRST-SDSS (Best & Heckman 2012) and VLA-COSMOS catalog, respectively. Middle: 0.5−2 keV AGN luminosity () as a function of redshift. The red-filled circle with error bar represents the break luminosity at 0.5−2 keV obtained from Hasinger et al. (2005). Bottom: 12 μm luminosity L_12 μm (erg s⁻¹) as a function of redshift. The k-correction is made by assuming the AGN SED of Mullaney et al. (2011). The red filled circle with error bar represents the break luminosity estimated from the IR AGN studies (Delvecchio et al. 2014).