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    A Southern-Sky Total Intensity Source Catalogue at 2.3 GHz from S-Band Polarisation All-Sky Survey Data

    Access Status
    Fulltext not available
    Authors
    Meyers, B.
    Hurley-Walker, Natasha
    Hancock, Paul
    Franzen, Thomas
    Carretti, E.
    Staveley-Smith, L.
    Gaensler, B.
    Haverkorn, M.
    Poppi, S.
    Date
    2017
    Type
    Journal Article
    
    Metadata
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    Citation
    Meyers, B. and Hurley-Walker, N. and Hancock, P. and Franzen, T. and Carretti, E. and Staveley-Smith, L. and Gaensler, B. et al. 2017. A Southern-Sky Total Intensity Source Catalogue at 2.3 GHz from S-Band Polarisation All-Sky Survey Data. Publications of the Astronomical Society of Australia.
    Source Title
    Publications of the Astronomical Society of Australia
    DOI
    10.1017/pasa.2017.5
    ISSN
    1323-3580
    School
    Curtin Institute of Radio Astronomy (Physics)
    URI
    http://hdl.handle.net/20.500.11937/52160
    Collection
    • Curtin Research Publications
    Abstract

    Copyright © Astronomical Society of Australia 2017The S-band Polarisation All-Sky Survey has observed the entire southern sky using the 64-m Parkes radio telescope at 2.3 GHz with an effective bandwidth of 184 MHz. The surveyed sky area covers all declinations d ? 0°. To analyse compact sources, the survey data have been re-processed to produce a set of 107 Stokes I maps with 10.75 arcmin resolution and the large scale emission contribution filtered out. In this paper, we use these Stokes I images to create a total intensity southern-sky extragalactic source catalogue at 2.3 GHz. The source catalogue contains 23 389 sources and covers a sky area of 16 600 deg2, excluding the Galactic plane for latitudes |b| < 10°. Approximately, 8% of catalogued sources are resolved. S-band Polarisation All-Sky Survey source positions are typically accurate to within 35 arcsec. At a flux density of 225 mJy, the S-band Polarisation All-Sky Survey source catalogue is more than 95% complete, and ~ 94% of S-band Polarisation All-Sky Survey sources brighter than 500 mJy beam-1 have a counterpart at lower frequencies.

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