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dc.contributor.authorBurke-Spolaor, S.
dc.contributor.authorEkers, Ronald
dc.contributor.authorMassardi, M.
dc.contributor.authorMurphy, T.
dc.contributor.authorPartridge, B.
dc.contributor.authorRicci, R.
dc.contributor.authorSadler, E.
dc.date.accessioned2017-01-30T11:38:18Z
dc.date.available2017-01-30T11:38:18Z
dc.date.created2016-09-12T08:37:06Z
dc.date.issued2009
dc.identifier.citationBurke-Spolaor, S. and Ekers, R. and Massardi, M. and Murphy, T. and Partridge, B. and Ricci, R. and Sadler, E. 2009. Wide-field imaging and polarimetry for the biggest and brightest in the 20-GHz southern sky. Monthly Notices of the Royal Astronomical Society. 395 (1): pp. 504-517.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/13632
dc.identifier.doi10.1111/j.1365-2966.2009.14556.x
dc.description.abstract

We present the wide-field imaging and polarimetry at ? = 20 GHz of seven most extended, bright (Stotal = 0.50 Jy), high-frequency selected radio sources in the southern sky with declinations d < -30°. Accompanying the data are brief reviews of the literature for each source. The results presented here aid in the statistical completeness of the Australia Telescope 20-GHz Survey: the Bright Source Sample. The data are of crucial interest for future cosmic microwave background missions as a collection of information about candidate calibrator sources. We were able to obtain data for seven of the nine sources identified by our selection criteria. We report that Pictor A is thus far the best extragalactic calibrator candidate for the Low Frequency Instrument of the Planck European Space Agency mission due to its high level of integrated polarized flux density (~0.50 ± 0.06 Jy) on a scale of 10 arcmin. Six out of the seven sources have a clearly detected compact radio core in our images, with either a null detection or less than 2 per cent detection of polarized emission from the nuclei. Most sources with detected jets have magnetic field alignments running in a longitudinal configuration, however, PKS 1333-33 exhibits transverse fields and an orthogonal change in field geometry from nucleus to jets. © 2009 RAS.

dc.publisherOxford University Press
dc.titleWide-field imaging and polarimetry for the biggest and brightest in the 20-GHz southern sky
dc.typeJournal Article
dcterms.source.volume395
dcterms.source.number1
dcterms.source.startPage504
dcterms.source.endPage517
dcterms.source.issn0035-8711
dcterms.source.titleMonthly Notices of the Royal Astronomical Society
curtin.departmentCurtin Institute of Radio Astronomy (Engineering)
curtin.accessStatusOpen access via publisher


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