  Results from the 327-MHz Giant Meterwave Radio Telescope (GMRT) observations
of four fields - three fields containing Galactic supernova remnants (SNRs)
(G001.4-0.1, G003.8+0.3, and G356.3-1.5) and one field containing a candidate
SNR (G004.2+0.0), are reported in this paper. These fields were selected from
the 843-MHz survey conducted by Gray (1994b) using the Molonglo Synthesis
Telescope (MOST). All the three SNRs are detected in the GMRT images.
Significant amount of thermal emission is seen at the location of the candidate
SNR, and the GMRT image shows a discrete source of emission which is consistent
with it being a flat spectrum thermal source. An incomplete arc of emission
with a compact central source detected in one of the fields, is coincident with
the extended OH(1720 MHz) emission reported earlier. Possible implications of
this morphology and correlation with the OH(1720 MHz) emission are also
discussed.
