Individual optical variability of Active Galactic Nuclei from the MEXSAS2 sample

no code implementations • 12 Oct 2020 • M. Laurenti, F. Vagnetti, R. Middei, M. Paolillo

We model the SF as a power-law, $\text{SF}(\tau)=A\,(\tau/\tau_0)^\gamma$, and we compute its variability parameters.

Astrophysics of Galaxies