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Finding the population of pulsars in the Milky Way galaxy requires a knowledge of the parameters and limitations of the various surveys made with different instruments and in different regions of the sky. We list the available survey data and show how models of the galactic population can be compared with the observational data, allowing estimates of pulsar birthrate and lifetime. Determination of accurate positions of individual pulsars require a Solar System ephemeris and a complex geometrical computation. Binary pulsar orbits display reletivistic effects which can be measured with remarkable precision to yield parameters of orbits and checks on relativistic theory.
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