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.Comment: 5 pages,2 figures, proceedings of 'Fermi & Jansky:Our Evolving
Understanding of AGN
