Slow pulsars from the STScI/NAIC drift scan search

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dc.creatorXilouris, K.
dc.creatorFruchter, A.
dc.creatorLorimer, D. R.
dc.creatorEder, J.
dc.creatorVazquez, A.
dc.date1999-11-02
dc.date1999-11-10
dc.date.accessioned2026-07-07T02:34:11Z
dc.date.available2026-07-07T02:34:11Z
dc.descriptionThe unique sensitivity of the Arecibo telescope at 430 MHz motivated a drift scan search of the visible sky divided up into eight declination strips. Based on an analysis of the data collected in the region assigned to us, eight new long-period pulsars have so far been discovered.
dc.description2 pages, 1 figure, to appear in the proceedings of the IAU 177 meeting - Pulsar Astronomy 2000 and beyond, replaced typos
dc.identifierhttps://arxiv.org/abs/astro-ph/9911012
dc.identifierhttp://arxiv.org/abs/astro-ph/9911012
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15144
dc.subjectAstrophysics
dc.titleSlow pulsars from the STScI/NAIC drift scan search
dc.typetext

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