The Southern Hemisphere VLBI Experiment Program, SHEVE

D.L. Jauncey, J.E. Reynolds, A.K. Tzioumis, R.H. Ferris, R.P. Norris, M.W. Sinclair, V. Migenes, R.G. Gough, R.M. Wark, R.A. Preston, D.L. Meier, D.W. Murphy, D.L. Jones, D.W. Hoard, M.E. St John, L. Skjerve, E.A. King, P.M. Mcculloch, J.E.J. Lovell, P.A. HamiltonM.E. Costa, David Blair, P. Edwards, R.W. Clay, D. Campbell-Wilson, S.W. Amy, W.B. Mcadam, G.L. White, P.A. Jones, G.D. Nicholson

    Research output: Chapter in Book/Conference paperChapterpeer-review

    Abstract

    The Southern Hemisphere VLBI Experiment (SHEVE) program is aimed at producing high-resolution images of southern radio sources. The radio telescopes of the present SHEVE array are described below and some recent results presented.
    Original languageEnglish
    Title of host publicationVery High Angular Resolution Imaging
    EditorsJ.G. Robertson, W.F. Tango
    Place of PublicationDordrecht
    PublisherInternational Astronomical Union
    Pages131-134
    Publication statusPublished - 1994

    Fingerprint

    Dive into the research topics of 'The Southern Hemisphere VLBI Experiment Program, SHEVE'. Together they form a unique fingerprint.

    Cite this