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- W2004383012 abstract "We present optical monitoring between 1994 February and 1997 December of 10 γ-ray-loud blazars included in our blazar monitoring program. Most of the monitored objects show significant rapid variations. The typical minimum variability timescale in the optical range is about 1 hour. We have analyzed the relationships between optical variability and γ-ray variability, and discussed theoretical models for the γ-ray-loud blazar emission." @default.
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- W2004383012 date "1999-09-10" @default.
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- W2004383012 title "Optical Monitoring Sample of the GeV Gamma‐Ray–loud Blazars" @default.
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- W2004383012 doi "https://doi.org/10.1086/307673" @default.
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