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Long-term Timing of 374 Pulsars

Published online by Cambridge University Press:  19 July 2016

G. Hobbs ,
A. Lyne  and
M. Kramer
G. Hobbs
Affiliation:
Australia Telescope National Facility — CSIRO, P.O. Box 76, Epping NSW 1710, Australia
A. Lyne
Affiliation:
Jodrell Bank Observatory, University of Manchester, Macclesfield, Cheshire SK11 9DL, UK
M. Kramer
Affiliation:
Jodrell Bank Observatory, University of Manchester, Macclesfield, Cheshire SK11 9DL, UK

Abstract

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We have analyzed the arrival times for 374 pulsars that have been observed for more than six years using the 76-m Lovell telescope at Jodrell Bank Observatory. Here we present a qualitative analysis of structures seen in the timing residuals.

Type
Part 10: Radio Pulsar Timing
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 431 - 432
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Downs, G. S., & Reichley, P. E. 1983, ApJS, 53, 169.Google Scholar