  In this work, we present the results from a study using the Giant Meterwave
Radio Telescope (GMRT) to search for radio {emission} from planets around three
evolved stars namely $\alpha$~Tau, $\beta$~UMi, and $\beta$~Gem. Both
$\alpha$~Tau and $\beta$~UMi host massive $\sim$ 6 $M_J$ mass planets at about
$\sim$1.4 au from the central star, while $\beta$~Gem is host to a 2.9 $M_J$
mass planet at 1.7 au from the host star. We observe $\alpha$~Tau and $\beta$~
UMi at two u(upgraded)GMRT bands; band~3 (250-500~MHz) and band~4
(550-900~MHz). We also analyzed the archival observations from $\beta$ Gem at
150~MHz from GMRT. We did not detect any radio signals from these systems. At
400~MHz, the 3$\sigma$ upper limit is 87 $\mu$Jy/beam for $\alpha$~Tau~{b} and
77.4 $\mu$Jy/beam for $\beta$~UMi~{b}. From our observations at 650~MHz, we
place a 3$\sigma$ upper limit of 28.2 $\mu$Jy/beam for $\alpha$~Tau~b and 33.6
$\mu$Jy/beam for $\beta$~UMi~b. For $\beta$ Gem b, at 150~MHz, we place an
upper limit of 2.5 mJy. At 400~MHz and 650~MHz, our observations are the
deepest radio images for any exoplanetary system.
