  We present wide area UBRI photometry for globular clusters around the Leo
group galaxy NGC 3379. Globular cluster candidates are selected from their
B-band magnitudes and their (U-B)o vs (B-I)o colours. A colour-colour selection
region was defined from photometry of the Milky Way and M31 globular cluster
systems. We detect 133 globular cluster candidates which, supports previous
claims of a low specific frequency for NGC 3379. The Milky Way and M31 reveal
blue and red subpopulations, with (U-B)o and (B-I)o colours indicating mean
metallicities similar to those expected based on previous spectroscopic work.
The stellar population models of Maraston (2003) and Brocato etal (2000) are
consistent with both subpopulations being old, and with metallicities of [Fe/H]
\~ -1.5 and -0.6 for the blue and red subpopulations respectively. The models
of Worthey (1994) do not reproduce the (U-B)o colours of the red (metal-rich)
subpopulation for any modelled age. For NGC 3379 we detect a blue subpopulation
with similar colours and presumably age/metallicity, to that of the Milky Way
and M31 globular cluster systems. The red subpopulation is less well defined,
perhaps due to increased photometric errors, but indicates a mean metallicity
of [Fe/H] ~ -0.6.
