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Long-Term Multiwavelength Studies of High-Redshift Blazar 0836+710Following gamma-ray flaring activity of high-redshift (z=2.218) blazar 0836+710 in 2011, we have assembled a long-term multiwavelength study of this object. Although this source is monitored regularly by radio telescopes and the Fermi Large Area Telescope, its coverage at other wavelengths is limited. The optical flux appears generally correlated with the gamma-ray flux, while little variability has been seen at X-ray energies. The gamma-ray/radio correlation is complex compared to some other blazars. As for many blazars, the largest variability is seen at gamma-ray wavelengths.
Document ID
20130013610
Acquisition Source
Goddard Space Flight Center
Document Type
Presentation
Authors
Thompson, D. J. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Akyuz, A. (Cukurova Univ. Adana, Turkey)
Donato, D. (Maryland Univ. College Park, MD, United States)
Perkins, J. S. (Maryland Univ. Baltimore County Baltimore, MD, United States)
Larsson, S. (Stockholm Univ. Sweden)
Sokolovsky, K.
Fuhrmann, L. (Max-Planck-Inst. fuer Radioastronomie Bonn, Germany)
Kurtanidze, O. (Abastumani Astrophysical Observatory Georgia, Russian Federation)
Date Acquired
August 27, 2013
Publication Date
October 28, 2012
Subject Category
Astronomy
Report/Patent Number
GSFC-E-DAA-TN7014
Meeting Information
Meeting: 4th International Fermi Symposium
Location: Monterey, CA
Country: United States
Start Date: October 28, 2012
End Date: November 2, 2012
Sponsors: NASA Goddard Space Flight Center
Funding Number(s)
CONTRACT_GRANT: NNG06EO90A
Distribution Limits
Public
Copyright
Public Use Permitted.

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