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• W2017110852 abstract "We present results of a photometric CCD study of the incidence of microvariability in the optical emission of a sample of 20 blazars detected at gamma-ray energies by the EGRET instrument of the Compton Gamma-Ray Observatory. We have observed strong outbursts in some sources, but many others displayed no significant variability on timescales of hours. The typical minimum timescale is found to be of ~several hours, not tens of minutes as claimed by some authors. The duty cycle for optical intranight microvariations of gamma-ray blazars, as estimated from our observations, seems to be ~50%, lower than what is usually assumed. For night-to-night variations, instead, the duty cycle approaches that observed in radio-selected BL Lacs and flat-spectrum radio quasars (i.e. ~70%)." @default.
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• W2017110852 date "2002-07-12" @default.
• W2017110852 modified "2023-10-01" @default.
• W2017110852 title "Optical microvariability of EGRET blazars" @default.
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• W2017110852 doi "https://doi.org/10.1051/0004-6361:20020743" @default.
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