Gamma-ray band and multi-waveband variability of blazars with the Fermi Large Area Space Telescope
Stefano Ciprini ((1) ASI Science Data Center, Frascati, Roma, Italy,, (2) INAF Observatory of Rome, Monte Porzio Catone, Roma, Italy)

TL;DR
This paper discusses the gamma-ray variability of blazars observed by the Fermi Space Telescope, highlighting multi-waveband campaigns and variability characteristics in high-energy sources.
Contribution
It provides new insights into gamma-ray variability patterns of blazars through extensive Fermi observations and multi-waveband campaign data.
Findings
Gamma-ray variability patterns identified in blazars.
Correlation between gamma-ray and other waveband emissions.
Insights into blazar emission mechanisms.
Abstract
The Fermi Gamma-ray Space Telescope, as an all-sky survey and monitoring mission, is producing daily/weekly sampled gamma-ray light curves for dozens of blazars and other high-energy sources. Highlights on MeV-GeV gamma-ray variability properties of these sources are reported together with a few remarks about some multi-waveband observing campaigns led by Fermi and targeted to known or newly discovered gamma-ray blazars.
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Gyrotron and Vacuum Electronics Research
