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Flaring Activity from S5 0836+71 (4C71.07): What Can We Learn with Limited Multiwavelength Coverage?After a long period of quiescence in gamma rays, blazar S5 0836+71 (4C71.07) flared in the Spring of 2011. We found only limited multiwavelength coverage of the source. An indication of correlated optical/gamma-ray variability is not surprising for a FSRQ like this one. Radio observations at high frequencies, however, had seen a flare in late 2010, with no apparent related gamma-ray activity. This case seems to differ from the traditional pattern of finding gamma-ray flares during times of rising radio emission.
Document ID
20120001868
Acquisition Source
Goddard Space Flight Center
Document Type
Abstract
Authors
Thompson, D. J. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Donato, D. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Akyuz, A. (Cukurova Univ. Adana, Turkey)
Fuhrmann, L. (Max-Planck-Inst. fuer Radioastronomie Bonn, Germany)
Sokolovsky, K. (Max-Planck-Inst. fuer Radioastronomie Bonn, Germany)
Kurtanidze, O. (Abastumani Astrophysical Observatory Georgia, Russian Federation)
Date Acquired
August 25, 2013
Publication Date
November 10, 2011
Subject Category
Astrophysics
Report/Patent Number
GSFC.ABS.5553.2011
Report Number: GSFC.ABS.5553.2011
Meeting Information
Meeting: Fermi and Jansky: Our Evolving Understanding of AGN
Location: St. Michaels, MD
Country: United States
Start Date: November 10, 2011
End Date: November 12, 2011
Sponsors: NASA Goddard Space Flight Center
Distribution Limits
Public
Copyright
Public Use Permitted.

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