A Fast Search Technique for Binary Pulsars

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dc.creatorRansom, Scott M.
dc.date1999-11-05
dc.date.accessioned2026-07-07T02:34:14Z
dc.date.available2026-07-07T02:34:14Z
dc.descriptionI 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 (P_orb <~ 5 h).
dc.description2 pages, 4 Postscript figures, uses newpasp.sty. To appear in the proceedings of the IAU 177 meeting - Pulsar Astronomy 2000 and Beyond
dc.identifierhttps://arxiv.org/abs/astro-ph/9911073
dc.identifierhttp://arxiv.org/abs/astro-ph/9911073
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15164
dc.subjectAstrophysics
dc.titleA Fast Search Technique for Binary Pulsars
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