The Parkes multi-beam pulsar survey - I. Observing and data analysis systems, discovery and timing of 100 pulsars

@article{Manchester2001ThePM,
  title={The Parkes multi-beam pulsar survey - I. Observing and data analysis systems, discovery and timing of 100 pulsars},
  author={Richard N. Manchester and Andrew G. Lyne and Fernando Camilo and Jon F. Bell and Victoria M. Kaspi and Nicolo' D'Amico and N. P. F. McKay and Fronefield Crawford and Ingrid H. Stairs and Andrea Possenti and Michael Kramer and D. C. Sheppard},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2001},
  volume={328},
  pages={17-35}
}
limiting flux density of the survey is about 0.2 mJy. At shorter or longer periods or higher dispersions, the sensitivity is reduced. Timing observations are carried out for pulsars discovered in the survey for 12‐18 months after confirmation to obtain accurate positions, spin parameters, dispersion measures, pulse shapes and mean flux densities. The survey is proving to be extremely successful, with more than 600 pulsars discovered so far. We expect that, when complete, this one survey will… 

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