A census of Fermi gamma-ray light curves shows FSRQs are more variable than BL Lacs, BCUs resemble BL Lacs, flux distributions are often log-normal, and PSD slopes are generally flat.
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Comprehensive Variability Analysis of Blazars Using Fermi Light Curves Across Multiple Timescales
A census of Fermi gamma-ray light curves shows FSRQs are more variable than BL Lacs, BCUs resemble BL Lacs, flux distributions are often log-normal, and PSD slopes are generally flat.