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The VSOP Survey Program

Published online by Cambridge University Press:  13 May 2016

J. E. J. Lovell ,
E.B. Fomalont ,
G.A. Moellenbrock ,
S. Horiuchi ,
H. Hirabayashi ,
W.K. Scott  and
R. Dodson
J. E. J. Lovell
Affiliation:
Australia Telescope National Facility, Epping, New South Wales 2122, Australia
E.B. Fomalont
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA, USA
G.A. Moellenbrock
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA, USA
S. Horiuchi
Affiliation:
Institute of Space and Astronautical Science, Sagamihara, Kanagawa 229-8510
H. Hirabayashi
Affiliation:
Institute of Space and Astronautical Science, Sagamihara, Kanagawa 229-8510
W.K. Scott
Affiliation:
University of Calgary, Calgary, Alberta, T2N 1N4, Canada
R. Dodson
Affiliation:
University of Tasmania, Hobart, Tasmania 7000, Australia

Abstract

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The VSOP Survey Program contains 402 bright, small diameter extragalactic radio sources. Pre-launch observations indicated that 113 sources were probably undetectable on space-ground baselines, and so VSOP observations are being undertaken at 5 GHz of the remaining 289 sources. Progress to date is described.

Type
The Inner Regions of Galaxies
Information
Symposium - International Astronomical Union , Volume 205: Galaxies and their Constituents at the Highest Angular Resolutions , 2001 , pp. 122 - 123
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

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Hirabayashi, H., Fomalont, E.B. et al. 2000b, PASJ in press.Google Scholar
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Moellenbrock, G.A., et al. 2000, in Astrophysical Phenomena Revealed by Space VLBI, ed Hirabayashi, H., Edwards, P.G., Murphy, D.W. (ISAS, Sagamihara) p177.Google Scholar
Murata, Y., Hirabayashi, H., Edwards, P.G. 2001, these proceedings.Google Scholar