We have conducted a pulsar survey of intermediate Galactic latitudes ( 5 \hbox { $ { } ^ { \circ } $ } < |b| < 15 \hbox { $ { } ^ { \circ } $ } ) at 20 cm .
The survey has been highly successful , discovering 58 new pulsars , eight of which are recycled , in only \sim 14 days of integration time .
One pulsar has a very narrow ( 2 \hbox { $ { } ^ { \circ } $ } FWHM ) average profile for the pulsar ’ s period ( 278 ms ) .
The six new recycled binary systems provide valuable information on the formation of white dwarf pulsar binaries .
Two systems have massive white dwarf companions ( > 0.57 M _ { \odot } and > 1.2 M _ { \odot } ) , while another has a low mass ( \sim 0.2 M _ { \odot } ) companion in a 23.3-d orbit , residing the well-known orbital period “ gap ” .