The Parkes Multibeam Pulsar Survey

Simple item page
dc.creatorCamilo, F.
dc.creatorLyne, A. G.
dc.creatorManchester, R. N.
dc.creatorBell, J. F.
dc.creatorKaspi, V. M.
dc.creatorD'Amico, N.
dc.creatorMcKay, N. P. F.
dc.creatorCrawford, F.
dc.creatorStairs, I. H.
dc.creatorMorris, D. J.
dc.creatorSheppard, D. C.
dc.creatorPossenti, A.
dc.date1999-11-10
dc.date.accessioned2026-07-07T02:34:20Z
dc.date.available2026-07-07T02:34:20Z
dc.descriptionThe Parkes multibeam pulsar survey uses a 13-element receiver operating at a wavelength of 20 cm to survey the inner Galactic plane with remarkable sensitivity. To date we have collected and analyzed data from 45% of the survey region (|b| < 5 deg.; 260 deg. < l < 50 deg.), and have discovered 440 pulsars, in addition to re-detecting 190 previously known ones. Most of the newly discovered pulsars are at great distances, as inferred from a median dispersion measure (DM) of 400 pc/cm^3.
dc.description6 pages, 8 included figures, to be published in proceedings of "Pulsar Astronomy -- 2000 and Beyond", ASP Conf. Ser
dc.identifierhttps://arxiv.org/abs/astro-ph/9911185
dc.identifierhttp://arxiv.org/abs/astro-ph/9911185
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15203
dc.subjectAstrophysics
dc.titleThe Parkes Multibeam Pulsar Survey
dc.typetext

Files

Collections

arXiv