SHMR for central AGNs and their control galaxies. For our results, those halo masses derived by M1 are given by diamonds with error bars, while those derived by M2 are given by dots with error bars. For comparison, we also show the SHMR in the literature, obtained by using various methods, including galaxy group catalog (Yang et al. 2009), abundance matching (see e.g. Moster et al. 2010; Behroozi et al. 2019), conditional luminosity function (Kravtsov et al. 2018), and weak lensing (Leauthaud et al. 2012).