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Spectral index properties of milliJansky radio sources

dc.contributor.authorRandall, K E
dc.contributor.authorHopkins, Andrew M.
dc.contributor.authorNorris, R P
dc.contributor.authorZinn, P.-C.
dc.contributor.authorMiddelberg, E
dc.contributor.authorMao, M Y
dc.contributor.authorSharp, Robert
dc.date.accessioned2015-12-10T23:26:09Z
dc.date.issued2012
dc.date.updated2016-02-24T08:47:29Z
dc.description.abstractAt the faintest radio flux densities (S1.4 < 10mJy), conflicting results have arisen regarding whether there is a flattening of the average spectral index between a low radio frequency (325 or 610MHz) and, for example, 1.4GHz. We present a new catalogue of 843-MHz radio sources in the European Large Area ISO Survey-South 1 field, which contains the sources, their Australia Telescope Large Area Survey (ATLAS) counterparts and the spectral index distribution of the sources as a function of flux density. We do not find any statistically significant evidence for a trend towards flatter spectral indices with decreasing flux density. We then investigate the spectral index distribution with redshift for those sources with reliable redshifts and explore the infrared properties. An initial sample of faint compact steep-spectrum sources in ATLAS are also presented, with a brief overview of their properties.
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/67643
dc.publisherBlackwell Publishing Ltd
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Catalogues; Galaxies: active; Galaxies: evolution; Radio continuum: galaxies
dc.titleSpectral index properties of milliJansky radio sources
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage1660
local.bibliographicCitation.startpage1644
local.contributor.affiliationRandall, K E, University of Sydney
local.contributor.affiliationHopkins, Andrew M., Australian Astronomical Observatory
local.contributor.affiliationNorris, R P, CSIRO Astronomy and Space Science (CASS)
local.contributor.affiliationZinn, P.-C., Ruhr-Universität Bochum
local.contributor.affiliationMiddelberg, E, Ruhr-Universität Bochum
local.contributor.affiliationMao, M Y, CSIRO Astronomy and Space Science
local.contributor.affiliationSharp, Robert, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidSharp, Robert, u4954956
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB1492
local.identifier.citationvolume421
local.identifier.doi10.1111/j.1365-2966.2012.20422.x
local.identifier.scopusID2-s2.0-84858449970
local.identifier.thomsonID000302695600056
local.type.statusPublished Version

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