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The Parkes Multibeam Pulsar Survey

F. Camilo·A. G. Lyne·R. N. Manchester·J. F. Bell·V. M. Kaspi·N. D'Amico·N. P. F. McKay·F. Crawford·I. H. Stairs·D. J. Morris·D. C. Sheppard·A. Possenti
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Abstract

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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F. Camilo, A. G. Lyne, R. N. Manchester, J. F. Bell, V. M. Kaspi, N. D'Amico, N. P. F. McKay, F. Crawford, I. H. Stairs, D. J. Morris, D. C. Sheppard, A. Possenti. 1999-11-10. The Parkes Multibeam Pulsar Survey. https://arxiv.org/abs/astro-ph/9911185

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