  We have used the 150 MHz radio continuum survey (TGSS ADR) from the Giant
Metrewave Radio Telescope (GMRT) to search for phase-averaged emission toward
all well-localized radio pulsars north of -53deg Declination. We detect
emission toward 200 pulsars with high confidence (>=5-sigma) and another 88
pulsars at fainter levels. We show that most of our identifications are likely
from pulsars, except for a small number where the measured flux density is
confused by an associated supernova or pulsar-wind nebula, or a globular
cluster. We investigate the radio properties of the 150 MHz sample and we find
an unusually high number of gamma-ray binary millisecond pulsars with very
steep spectral indices. We also note a discrepancy in the measured flux
densities between GMRT and LOFAR pulsar samples, suggesting that the flux
density scale for the LOFAR pulsar sample may be in error by approximately a
factor two. We carry out a separate search of 30 well-localized gamma-ray,
radio-quiet pulsars in an effort to detect a widening of the radio beam into
the line-of-sight at lower frequencies. No steep spectrum emission was detected
either toward individual pulsars or in a weighted stack of all 30 images.
