CL-AGNs follow the usual M_BH-sigma_* and M_BH-M_* scaling relations of inactive galaxies with typical host stellar populations, indicating they are a phase of normal AGN activity rather than a distinct population.
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Changing-Look Active Galactic Nuclei in SDSS-V: Host-Galaxy Properties and Black-Hole Scaling Relations
CL-AGNs follow the usual M_BH-sigma_* and M_BH-M_* scaling relations of inactive galaxies with typical host stellar populations, indicating they are a phase of normal AGN activity rather than a distinct population.