VAR-PZ uses DRW-modeled variability to create photo-z priors that reduce catastrophic outliers in AGN redshift estimates from 32% to below 7% when combined with SED fitting, validated on SDSS data and LSST simulations.
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Spectral monitoring indicates NGC 3786's changing-look AGN transition results from torus covering factor variations driven by Eddington ratio and accretion mode changes.
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VAR-PZ: Constraining the Photometric Redshifts of Quasars using Variability
VAR-PZ uses DRW-modeled variability to create photo-z priors that reduce catastrophic outliers in AGN redshift estimates from 32% to below 7% when combined with SED fitting, validated on SDSS data and LSST simulations.
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The Changing-look Phenomenon Accompanied by an Accretion Mode Transition in NGC 3786
Spectral monitoring indicates NGC 3786's changing-look AGN transition results from torus covering factor variations driven by Eddington ratio and accretion mode changes.