  We present results from a search for pulsars in globular clusters, including
the discovery of a new millisecond pulsar in the stellar cluster GLIMPSE-C01.
We searched for low frequency radio sources within 97 globular clusters using
images from the VLA Low-band Ionosphere and Transient Experiment (VLITE) and
epochs 1 and 2 of the VLITE Commensal Sky Survey (VCSS). We discovered 10
sources in our search area, four more than expected from extragalactic source
counts at our sensitivity limits. The strongest pulsar candidate was a point
source found in GLIMPSE-C01 with a spectral index ~ -2.6, and we present
additional measurements at 0.675 and 1.25 GHz from the GMRT and 1.52 GHz from
the VLA which confirm the spectral index. Using archival Green Bank Telescope
S-band data from 2005, we detect a binary pulsar with a spin period of 19.78 ms
within the cluster. Although we cannot confirm that this pulsar is at the same
position as the steep spectrum source using the existing data, the pulse flux
is consistent with the predicted flux density from other frequencies, making it
a probable match. The source also shows strong X-ray emission, indicative of a
higher magnetic field than most millisecond pulsars, suggesting that its
recycling was interrupted. We demonstrate that low frequency searches for steep
spectrum sources are an effective way to identify pulsar candidates,
particularly on sightlines with high dispersion.
