  Double-peaked emission line AGN (DPAGN) have been regarded as binary black
hole candidates. We present here results from parsec-scale radio observations
with the Very Long Baseline Array (VLBA) of five DPAGN belonging to the KISSR
sample of emission-line galaxies. This work concludes our pilot study of nine
type 2 Seyfert and LINER DPAGN from the KISSR sample. In the nine sources, dual
compact cores are only detected in the "offset AGN", KISSR 102. The overall
incidence of jets however, in the eight sources detected with the VLBA, is
$\ge$60%. We find a difference in the "missing flux density" going from the
Very Large Array (VLA) to VLBA scales between Seyferts and LINERs, with LINERs
showing less missing flux density on parsec-scales. Using the emission-line
modeling code, MAPPINGS III, we find that the emission lines are likely to be
influenced by jets in 5/9 sources. Jet-medium interaction is the likely cause
of the emission-line splitting observed in the SDSS spectra of these sources.
Jets in radio-quiet AGN are therefore energetically capable of influencing
their parsec- and kpc-scale environments, making them agents of "radio AGN
feedback", similar to radio-loud AGN.
