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We obtained radio observations of the symbiotic binary and known recurrentnova T Coronae Borealis following a period of increased activity in the opticaland X-ray bands. A comparison of our observations with those made prior to 2015indicates that the system is in a state of higher emission in the radio aswell. The spectral energy distributions are consistent with optically thickthermal bremsstrahlung emission from a photoionized source. Our observationsindicate that the system was in a state of increased ionization in thecompanion wind, possibly driven by an increase in accretion rate, with theradio photosphere located well outside the binary system.

T CrB: Radio Observations During the 2016--2017 "Super-Active" State