Probing Radio Emission in Seyfert Galaxies on Parsec- and
  Kiloparsec-scales
  Seyfert galaxies have traditionally been classified as radio-quiet active
galactic nuclei. A proper consideration of the nuclear optical emission however
proves that a majority of Seyferts are radio-loud. Kpc-scale radio
lobes/bubbles are in fact revealed in sensitive observations at low radio
frequencies of several Seyferts. Through the use of very long baseline
interferometry, we have been able to determine the direction of the
parsec-scale jets in some of these Seyfert galaxies. The misalignment between
the parsec-scale jets and the kpc-scale lobes that is typically observed, is
either suggestive of no connection between the two, or the presence of curved
jets that power the radio lobes. In this context, we briefly discuss our new
low radio frequency GMRT observations of two Seyfert galaxies with lobes.
