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Gamma-Ray Waveband and Multi-Waveband Variability of Blazars

Published online by Cambridge University Press:  20 April 2012

Stefano Ciprini
Stefano Ciprini*
Affiliation:
ASI Science Data Center, Frascati, Roma, Italy INAF Observatory of Rome, Monte Porzio Catone, Roma, Italy email: stefano.ciprini@asdc.asi.it
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Abstract

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The Fermi Gamma-ray Space Telescope, as an all-sky survey and monitoring mission, is producing well-sampled gamma-ray light curves for dozens of blazars and other high-energy sources. We report highlights of gamma-ray variability properties, and outline multi-frequency observing campaigns that are targeted to new or known blazars which emit gamma rays.

Keywords

surveyscataloguesgamma rays: observationsquasars: generalBL Lacertae objects: generalmethods: statisticalradiation mechanisms: nonthermal
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S285: New Horizons in Time-Domain Astronomy , September 2011 , pp. 121 - 124
Copyright
Copyright © International Astronomical Union 2012

References

Abdo, A. A., et al. , 2010a, ApJ, 722, 520CrossRefGoogle Scholar
Abdo, A. A., et al. , 2010b, ApJ, 710, 810CrossRefGoogle Scholar
Abdo, A. A., et al. , 2010c, Nature, 463, 919Google Scholar
Ackermann, M., et al. , 2010, ApJ, 721, 1383CrossRefGoogle Scholar
Ackermann, M., et al. , 2011, ApJ, in press (arXiv:1108.1420)Google Scholar
Atwood, W.B., et al. , 2009, ApJ, 697, 1071CrossRefGoogle Scholar