2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/15164I 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).2 pages, 4 Postscript figures, uses newpasp.sty. To appear in the proceedings of the IAU 177 meeting - Pulsar Astronomy 2000 and BeyondAstrophysicstext