Long-term multiwavelength studies of high-redshift blazar 0836+710
A. Akyüz, D. J. Thompson, D. Donato, J. S. Perkins, L. Fuhrmann, E. Angelakis, J. A. Zensus, S. Larsson, K. V. Sokolovsky, O. M. Kurtanidze
Abstract
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A. Akyüz, D. J. Thompson, D. Donato, J. S. Perkins, L. Fuhrmann, E. Angelakis, J. A. Zensus, S. Larsson, K. V. Sokolovsky, O. M. Kurtanidze
Abstract
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Aims. The observation of γ-ray flares from blazar 0836+710 in 2011, following a period of quiescence, offered an opportunity to study correlated activity at different wavelengths for a high-redshift (z = 2.218) active galactic nucleus.
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Aims. The observation of γ-ray flares from blazar 0836+710 in 2011, following a period of quiescence, offered an opportunity to study correlated activity at different wavelengths for a high-redshift (z = 2.218) active galactic nucleus.
Key concepts: Blazar, Astrophysics, Redshift, Physics, Active galactic nucleus, Fermi Gamma-ray Space Telescope, Gamma ray, Flare