The Molonglo Southern 4 Jy sample (MS4). II. ATCA imaging and optical identification

dc.creatorBurgess, A. M.
dc.creatorHunstead, R. W.
dc.date2005-12-23
dc.date.accessioned2026-07-07T11:25:08Z
dc.date.available2026-07-07T11:25:08Z
dc.descriptionOf the 228 sources in the Molonglo Southern 4 Jy Sample (MS4), the 133 with angular sizes < 35 arcsec have been imaged at 5 GHz at 2-4 arcsec resolution with the Australia Telescope Compact Array. More than 90% of the sample has been reliably optically identified, either on the plates of the UK Schmidt Southern Sky Survey or on R-band CCD images made with the Anglo-Australian Telescope. A subsample of 137 sources, the SMS4, defined to be a close southern equivalent of the northern 3CRR sample, was found to have global properties mostly consistent with the northern sample. Linear sizes of MS4 galaxies and quasars were found to be consistent with galaxy-quasar unification models of orientation and evolution.
dc.description102 pages; 6 figures in 21 Postscript files. To appear in Astronomical Journal. For higher-resolution versions of some figures, see http://www.physics.usyd.edu.au/astrop/rwh/ms4/
dc.identifierhttps://arxiv.org/abs/astro-ph/0512590
dc.identifierhttp://arxiv.org/abs/astro-ph/0512590
dc.identifierAstron.J.131:114-132,2006
dc.identifierdoi:10.1086/498679
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195415
dc.subjectAstrophysics
dc.titleThe Molonglo Southern 4 Jy sample (MS4). II. ATCA imaging and optical identification
dc.typetext

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