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The Parkes Multibeam Pulsar Survey

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arxiv astro-ph/9911185 v1 pith:YYDDA6M3 submitted 1999-11-10 astro-ph

F. Camilo , A. G. Lyne , R. N. Manchester , J. F. Bell , V. M. Kaspi , N. D'Amico , N. P. F. McKay , F. Crawford
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I. H. Stairs D. J. Morris D. C. Sheppard A. Possenti
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classification astro-ph
keywords surveydiscoveredmultibeamparkespulsarpulsarsadditionanalyzed
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The 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.

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