A Fast Search Technique for Binary Pulsars
Scott M. Ransom
Abstract
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).
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