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    The VSOP 5 GHz Active Galactic Nucleus Survey. II. Data Calibration and Imaging

    Access Status
    Open access via publisher
    Authors
    Lovell, J.
    Moellenbrock, G.
    Horiuchi, S.
    Fomalont, E.
    Scott, W.
    Hirabayashi, H.
    Dodson, R.
    Dougherty, S.
    Edwards, P.
    Frey, S.
    Gurvits, L.
    Lister, M.
    Murphy, D.
    Paragi, Z.
    Piner, B.
    Shen, Z.
    Taylor, A.
    Tingay, Steven
    Asaki, Y.
    Moffett, D.
    Murata, Y.
    Date
    2004
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Lovell, J and Moellenbrock, G and Horiuchi, S and Fomalont, E and Scott, W and Hirabayashi, H and Dodson, R et al. 2004. The VSOP 5 GHz Active Galactic Nucleus Survey. II. Data Calibration and Imaging. The Astrophysical Journal. 155 (1): pp. 27-31.
    Source Title
    The Astrophysical Journal
    DOI
    10.1086/424820
    ISSN
    0004637X
    Faculty
    Faculty of Science and Engineering
    Curtin Institute of Radio Astronomy
    Remarks

    Copyright © 2004 The American Astronomical Society ("AAS")-[The Astrophysical Journal (ApJ) Lovell, 2004 ApJS 155 (1), 27-31.]

    URI
    http://hdl.handle.net/20.500.11937/10928
    Collection
    • Curtin Research Publications
    Abstract

    The VLBI Space Observatory Programme (VSOP) mission is a Japanese-led project to study radio sources with sub-milliarcsecond angular resolution using an orbiting 8 m telescope, HALCA, and global arrays of Earth-based telescopes. Approximately 25% of the observing time has been devoted to a survey of compact active galactic nuclei (AGNs) at 5 GHz that are stronger than 1 Jy-the VSOP AGN Survey. This paper, the second in a series, describes the data calibration, source detection, self-calibration, imaging, and modeling and gives examples illustrating the problems specific to space VLBI. The VSOP Survey Web site, which contains all results and calibrated data, is described.

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