A criterion of |Δg| > 0.4 mag and |Δ(g-r)| > 0.2 mag detects photometric CL-AGN transitions in 9.6% of known hosts with 1.6% false positive rate from simulations.
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4 Pith papers cite this work. Polarity classification is still indexing.
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2026 4representative citing papers
Quasar light curves constrain short-term volatility η better than timescale τ in DRW models; hierarchical Bayesian fit on 570 curves shows volatility decreases with bolometric luminosity and rest wavelength.
Mass-scaled DRW damping timescales in AGNs follow a linear relation with black hole mass (slope 0.35-0.50) for both jetted and non-jetted sources, supporting universal accretion physics.
citing papers explorer
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Identifying Changing-Look AGN Transitions in Light Curve Data with the Zwicky Transient Facility
A criterion of |Δg| > 0.4 mag and |Δ(g-r)| > 0.2 mag detects photometric CL-AGN transitions in 9.6% of known hosts with 1.6% false positive rate from simulations.
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The Information Content of Quasar Variability Light Curves: How Well Can we Infer Stochastic Model Parameters?
Quasar light curves constrain short-term volatility η better than timescale τ in DRW models; hierarchical Bayesian fit on 570 curves shows volatility decreases with bolometric luminosity and rest wavelength.
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A universal relationship between the variability timescale and black hole mass in black hole jetted and non-jetted accreting systems
Mass-scaled DRW damping timescales in AGNs follow a linear relation with black hole mass (slope 0.35-0.50) for both jetted and non-jetted sources, supporting universal accretion physics.
- Optical Variability Structure Function of Low-Luminosity AGN using ATLAS Lightcurves