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The Southern Hemisphere VLBI Experiment (Sheve)

Published online by Cambridge University Press:  04 August 2017

R.A. Preston ,
D.L. Jauncey ,
A. Tsioumis ,
D.L. Meier ,
L.J. Skjerve ,
J. Ables ,
R. Batchelor ,
J. Faulkner ,
P.M. Hamilton  and
R. Haynes
...Show all authors
R.A. Preston
Affiliation:
1Jet Propulsion Laboratory, Pasadena, California
D.L. Jauncey
Affiliation:
2CSIRO, Sydney, Australia
A. Tsioumis
Affiliation:
3Sydney University, Sydney, Australia
D.L. Meier
Affiliation:
1Jet Propulsion Laboratory, Pasadena, California
L.J. Skjerve
Affiliation:
1Jet Propulsion Laboratory, Pasadena, California
J. Ables
Affiliation:
2CSIRO, Sydney, Australia
R. Batchelor
Affiliation:
2CSIRO, Sydney, Australia
J. Faulkner
Affiliation:
1Jet Propulsion Laboratory, Pasadena, California
P.M. Hamilton
Affiliation:
4University of Tasmania, Hobart, Australia
R. Haynes
Affiliation:
2CSIRO, Sydney, Australia
B. Johnson
Affiliation:
5Ford Aerospace and Communications Corporation, Goldstone, California
A. Louie
Affiliation:
1Jet Propulsion Laboratory, Pasadena, California
P. McCulloch
Affiliation:
4University of Tasmania, Hobart, Australia
G. Moorey
Affiliation:
2CSIRO, Sydney, Australia
D.D. Morabito
Affiliation:
1Jet Propulsion Laboratory, Pasadena, California
G. Nicolson
Affiliation:
6Hartebeesthoek Radio Astronomy Observatory, Johannesburg, South Africa
A.E. Niell
Affiliation:
1Jet Propulsion Laboratory, Pasadena, California
J.G. Robertson
Affiliation:
7Anglo-Australian Observatory, Sydney, Australia
G.W.R. Royle
Affiliation:
8Division of National Mapping, Canberra, Australia
M.A. Slade
Affiliation:
1Jet Propulsion Laboratory, Pasadena, California
O.B. Slee
Affiliation:
2CSIRO, Sydney, Australia
A. Watkinson
Affiliation:
3Sydney University, Sydney, Australia
A.E. Wehrle
Affiliation:
1Jet Propulsion Laboratory, Pasadena, California
A. Wright
Affiliation:
2CSIRO, Sydney, Australia

Extract

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The Southern Hemisphere VLBI Experiment (or SHEVE) was a joint US-Australian-South African venture with both astronomy and geodesy goals. The principle astronomy goal was to make models or maps of the following sources: at 2.3 GHz (with six antennas and 9 usable baselines) – Centaurus A (the nearest active galaxy), Circinus X-1 (a flaring binary), the VELA pulsar, and 26 other active galactic nuclei and quasars; at 8.4 GHz (only one baseline) – Centaurus A and the galactic center.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 110: VLBI and Compact Radio Sources , 1984 , pp. 67 - 69
Copyright
Copyright © Reidel 1984 

References

Preston, et al. 1983, Ap. J. (Letters), 266, 93.CrossRefGoogle Scholar
Phillips, and Mutel, 1981, Ap. J., 244, 19.CrossRefGoogle Scholar
Gubbay, J. S. et al. 1971, A. J., 76, 965.CrossRefGoogle Scholar