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The southern hemisphere VLBI experiment (SHEVE)Six radio telescopes were operated as the first southern hemisphere VLBI array in April and May 1982. Observations were made at 2.3 and 8.4 Ghz. This array produced VLBI images of 28 southern hemisphere radio sources, high accuracy VLBI geodesy between southern hemisphere sites, and sub-arcsecond radio astrometry of celestial sources south of declination -45 degrees. This paper discusses only the astrophysical aspects of the experiment.
Document ID
19890026367
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Preston, R. A. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Meier, D. L. (California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Jauncey, D. L. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Ables, J. (CSIRO Sydney, Australia)
Tzioumis, A. K. (Sydney, University Australia)
Date Acquired
August 14, 2013
Publication Date
January 1, 1988
Subject Category
Astronomy
Meeting Information
Meeting: IAU Symposium on the Impace of VLBI on Astrophysics and Geophysics
Location: Cambridge, MA
Country: United States
Start Date: May 10, 1987
End Date: May 15, 1987
Accession Number
89A13738
Distribution Limits
Public
Copyright
Other

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