THE PARKES SOUTHERN PULSAR SURVEY - II - FINAL RESULTS AND POPULATIONANALYSIS

A survey of the entire southern sky for millisecond and low-luminosity pulsars using the ATNF Parkes radio telescope has now been completed. The survey detected 298 pulsars, of which 101 were previously unknown . The new pulsars include 17 millisecond pulsars. This is the largest sample of both normal and millisecond pulsars detected in any survey. Combining our sample with other recent surveys in the Northern Hemisph ere, we present a statistical study of the populations of both normal and millisecond pulsars. We find that the improved statistics allow us to estimate the number and birth-rate of both types of pulsar down to a 400-MHz luminosity limit of 1 mJy kpc(2). The local surface densiti es of potentially observable normal pulsars and millisecond pulsars ar e both about 30 kpc(-2), corresponding to similar to 30 000 potentiall y observable pulsars of each type in the Galaxy. Once beaming effects are taken into consideration we estimate that the active population of normal pulsars is similar to 160 000. Although there is evidence for flattening of the luminosity function of normal pulsars, this is not e vident for millisecond pulsars which;probably have a substantial popul ation with luminosities below 1 mJy kpc(2). After correcting for beami ng effects, we estimate that a normal pulsar is born with a luminosity greater than 1 mJy kpc(2) between once every 60 and 330 yr in the Gal axy. The birth-rate of millisecond pulsars is at least 3 x 10(-6) yr(- 1) above the same luminosity limit. Modelling the observed transverse speeds of millisecond pulsars using a dynamical simulation, we find th eir mean birth velocity to be 130 +/- 30 km s(-)1, significantly lower than that of the normal pulsars.