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

Polarimetry of 600 pulsars from observations at 1.4 GHz with the Parkes radio telescope