Long-term multiwavelength studies of high-redshift blazar 0836+710
Akyuz, A.; Thompson, D. J.; Zensus, J. A.; Larsson, S.; Perkins, J. S.; Angelakis, E.; Fuhrmann, L.; Donato, D.; Sokolovsky, K.; Kurtanidze, O.
Turkey, United States, Germany, Sweden, Russia, Georgia
Abstract
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.
Methods: Optical and radio monitoring, plus Fermi-LAT γ-ray monitoring provided 2008-2012 coverage, while Swift offered auxiliary optical, ultraviolet, and X-ray information. Other contemporaneous observations were used to construct a broad-band spectral energy distribution.
Results: There is evidence of correlation but not a measurable lag between the optical and γ-ray flaring emission. In contrast, there is no clear correlation between radio and γ-ray activity, indicating radio emission regions that are unrelated to the parts of the jet that produce the γ rays. The γ-ray energy spectrum is unusual in showing a change of shape from a power law to a curved spectrum when going from the quiescent state to the active state.