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Timing the Parkes Multibeam Pulsars

Published online by Cambridge University Press:  12 April 2016

R. N. Manchester ,
A. G. Lyne ,
F. Camilo ,
V. M. Kaspi ,
I. H. Stairs ,
F. Crawford ,
D. J. Morris ,
J. F. Bell  and
N. D’Amico
R. N. Manchester
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping NSW 1710, Australia
A. G. Lyne
Affiliation:
University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, UK
F. Camilo
Affiliation:
University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, UK
V. M. Kaspi
Affiliation:
Center for Space Research, MIT, Cambridge MA 02139, USA
I. H. Stairs
Affiliation:
University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, UK
F. Crawford
Affiliation:
Center for Space Research, MIT, Cambridge MA 02139, USA
D. J. Morris
Affiliation:
University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, UK
J. F. Bell
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping NSW 1710, Australia
N. D’Amico
Affiliation:
Osservatorio Astronomico di Bologna, 40127 Bologna, Italy

Abstract

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Measurement of accurate positions, pulse periods and period derivatives is an essential follow-up to any pulsar survey. The procedures being used to obtain timing parameters for the pulsars discovered in the Parkes multibeam pulsar survey are described. Completed solutions have been obtained so far for about 80 pulsars. They show that the survey is preferentially finding pulsars with higher than average surface dipole magnetic fields. Eight pulsars have been shown to be members of binary systems and some of the more interesting results relating to these are presented.

Type
Part 2. Timing, General Relativity and Astrometry
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 49 - 54
Copyright
Copyright © Astronomical Society of the Pacific 2000

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