Assessment of stochastic and deterministic models of 6304 quasar lightcurves from SDSS Stripe 82
Rene Andrae, Dae-Won Kim, Coryn A.L. Bailer-Jones

TL;DR
This study compares over 20 stochastic and deterministic models to describe quasar light curves, finding the Ornstein-Uhlenbeck process to be the most effective for the majority of cases, thus confirming the stochastic nature of quasar variability.
Contribution
It provides a comprehensive Bayesian comparison of multiple models, establishing the Ornstein-Uhlenbeck process as the best fit for most quasar light curves in SDSS Stripe 82.
Findings
The OU process best describes 6023 out of 6304 light curves.
Composite OU/sinusoid models are dominant for brighter/bluer QSOs.
Many light curves show stochastic variance, not just mean variability.
Abstract
The optical light curves of many quasars show variations of tenths of a magnitude or more on time scales of months to years. This variation often cannot be described well by a simple deterministic model. We perform a Bayesian comparison of over 20 deterministic and stochastic models on 6304 QSO light curves in SDSS Stripe 82. We include the damped random walk (or Ornstein-Uhlenbeck [OU] process), a particular type of stochastic model which recent studies have focused on. Further models we consider are single and double sinusoids, multiple OU processes, higher order continuous autoregressive processes, and composite models. We find that only 29 out of 6304 QSO lightcurves are described significantly better by a deterministic model than a stochastic one. The OU process is an adequate description of the vast majority of cases (6023). Indeed, the OU process is the best single model for 3462…
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