  Over the past 13 years, the Parkes radio telescope has observed a large
number of pulsars using digital filterbank backends with high time and
frequency resolution and the capability for Stokes recording. Here we use
archival data to present polarimetry data at an observing frequency of 1.4 GHz
for 600 pulsars with spin-periods ranging from 0.036 to 8.5 s. We comment
briefly on some of the statistical implications from the data and highlight the
differences between pulsars with high and low spin-down energy. The dataset,
images and table of properties for all 600 pulsars are made available in a
public data archive maintained by the CSIRO.
