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In this work, we use the Jansky VLA Sky Survey (VLASS) to compile the firstsample of six radio-selected tidal disruption events (TDEs) with transientoptical counterparts. While we still lack the statistics to do detailedpopulation studies of radio-selected TDEs, we use these events to suggesttrends in host galaxy and optical light curve properties that may correlatewith the presence of radio emission, and hence can inform optically-selectedTDE radio follow-up campaigns. We find that radio-selected TDEs tend to havefaint and cool optical flares, as well as host galaxies with low SMBH masses.Our radio-selected TDEs also tend to have more energetic, larger radio emittingregions than radio-detected, optically-selected TDEs. We consider possibleexplanations for these trends, including by invoking super-Eddington accretionand enhanced circumnuclear media. Finally, we constrain the radio-emitting TDErate to be $\gtrsim 10$ Gpc$^{-3}$ yr$^{-1}$.

VLASS tidal disruption events with optical flares I: the sample and a comparison to optically-selected TDEs