  Globular clusters contain a unique pulsar population, with many exotic
systems that can form only in their dense stellar environments. The leap in
sensitivity of the upgraded Giant Metrewave Radio Telescope (uGMRT) in India,
especially at low radio frequencies ($<$ 1 GHz) has motivated a new search for
radio pulsars in a group of eight Southern globular clusters. We discovered PSR
J1835$-$3259B, a 1.83-ms pulsar in NGC 6652; this is in a near-circular wide
orbit of 28.7 hr with a low-mass ($ \sim 0.2 \, M_{\rm \odot}$) companion,
likely a Helium white dwarf. We derived a 10-year timing solution for this
system. We also present measurements of scattering, flux densities and spectral
indices for some of the previously known pulsars in these GCs. A significant
fraction of the pulsars in these clusters have steep spectral indices.
Additionally, we detected eight radio point sources not associated with any
known pulsar positions in the radio images. There are four newly identified
sources, three in NGC 6652 and one in NGC 6539, and one previously identified
source each in NGC 1851, NGC 6440, NGC 6544, and Terzan 5. Surprisingly, our
images show that our newly discovered pulsar, PSR J1835$-$3259B, is the
brightest pulsar in all GCs we have imaged; like other pulsars with broad
profiles (Terzan 5 C and O), its flux density in the radio images is much
larger than in its pulsations. This indicates that their pulsed emission is
only a fraction of their total emission. The detection of radio sources outside
the core radii but well within the tidal radii of these clusters show that
future GC surveys should complement the search analysis by using the imaging
capability of interferometers, and preferentially synthesize large number of
search beams in order to obtain a larger field of view.
