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arXiv · 1205.2238

Flaring Activity from 0836+710 (4C +71.07): What Can We Learn With Limited Multiwavelength Coverage?

A. Akyuz·D. J. Thompson·D. Donato·L. Fuhrmann·K. Sokolovsky·O. Kurtanidze
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Abstract

After a long period of quiescence in \gamma-rays, blazar 0836+710 (4C +71.07) 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 Flat Spectrum Radio Quasar (FSRQ) like this one. Radio observations at high frequencies, however, had seen a flare in 2010, well offset from possible \gamma-ray activity. The 2011 \gamma-ray activity comes during a period of rising radio emission, a pattern that has been seen since the EGRET era.

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A. Akyuz, D. J. Thompson, D. Donato, L. Fuhrmann, K. Sokolovsky, O. Kurtanidze. 2012-05-10. Flaring Activity from 0836+710 (4C +71.07): What Can We Learn With Limited Multiwavelength Coverage?. https://arxiv.org/abs/1205.2238

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