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The Parkes Multibeam Blind HI Survey

Published online by Cambridge University Press:  12 April 2016

R.L. Webster ,
V. Kilborn ,
J.C. O’Brien ,
L. Staveley-Smith ,
M.E. Putman  and
G. Banks
R.L. Webster
Affiliation:
School of Physics, University of Melbourne, Parkville, Vic, Australia, 3052
V. Kilborn
Affiliation:
School of Physics, University of Melbourne, Parkville, Vic, Australia, 3052
J.C. O’Brien
Affiliation:
School of Physics, University of Melbourne, Parkville, Vic, Australia, 3052
L. Staveley-Smith
Affiliation:
Australia Telescope National Facility, PO Box 76, Epping, NSW, Australia, 2121
M.E. Putman
Affiliation:
Mount Stromlo and Siding Springs Observatory, Australian National University, Weston Creek PO., ACT, Australia, 2611
G. Banks
Affiliation:
Department of Physics and Astronomy, University of Wales, Cardiff, PO Box 913, Cardiff, CF2 3YB, Wales, UK

Abstract

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A thirteen-beam HI receiver has been constructed for the Parkes radio telescope. When this instrument is used in active scanning mode, it can rapidly survey large areas of sky, with a relatively uniform sensitivity. The Multibeam Working Group, comprising about 30 astronomers from more than a dozen institutions, is undertaking a blind HI survey of the entire southern sky. The status of the survey is described, with some of the first scientific results.

Type
HI and QSO absorption lines
Information
International Astronomical Union Colloquium , Volume 171: The Low Surface Brightness Universe , 1999 , pp. 291 - 298
Copyright
Copyright © Astronomical Society of the Pacific 1999

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