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A Fast Search Technique for Binary Pulsars

Published online by Cambridge University Press:  12 April 2016

Scott M. Ransom
Scott M. Ransom*
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., MS 10, Cambridge, MA 02138, USA

Abstract

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I describe a computationally simple, efficient, and sensitive method to search long observations for pulsars in binary systems. The technique looks for orbitally induced sidebands in the power spectrum around a nominal spin frequency, enabling it to detect pulsars in high- or low-mass binaries with short orbital periods (Porb ≲ 5 h).

Type
Part 1. Searching for Pulsars
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 43 - 44
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Johnston, H.M. & Kulkarni, S.R. 1991, ApJ, 368, 504 CrossRefGoogle Scholar
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Ransom, S.M., Cordes, J.M. & Eikenberry, S.S. 2000, in preparation.Google Scholar