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dc.contributor.authorNorris, Ray P.
dc.contributor.authorHopkins, A. M.
dc.contributor.authorAfonso, J.
dc.contributor.authorBrown, S.
dc.contributor.authorCondon, J. J.
dc.contributor.authorDunne, L.
dc.contributor.authorFeain, I.
dc.contributor.authorHollow, R.
dc.contributor.authorJarvis, M.J.
dc.contributor.authorJohnston-Hollitt, M.
dc.contributor.authorLenc, E.
dc.contributor.authorMiddelberg, E.
dc.contributor.authorPadovani, P.
dc.contributor.authorPrandoni, I.
dc.contributor.authorRudnick, L.
dc.contributor.authorSeymour, N.
dc.contributor.authorUmana, G.
dc.contributor.authorAndernach, H.
dc.contributor.authorAlexander, D. M.
dc.contributor.authorAppleton, P. N.
dc.contributor.authorBacon, D.
dc.contributor.authorBanfield, J.
dc.contributor.authorBecker, W.
dc.contributor.authorBrown, M. J. I.
dc.contributor.authorCiliegi, P.
dc.contributor.authorJackson, C.
dc.contributor.authorEales, S.
dc.contributor.authorEdge, A. C.
dc.contributor.authorGaensler, B. M.
dc.contributor.authorGiovannini, G.
dc.contributor.authorHales, C. A.
dc.contributor.authorHancock, P.
dc.contributor.authorHuynh, M. T.
dc.contributor.authorIbar, E.
dc.contributor.authorIvison, R. J.
dc.contributor.authorKennicutt, R.
dc.contributor.authorKimball, Amy E.
dc.contributor.authorKoekemoer, A. M.
dc.contributor.authorKoribalski, B. S.
dc.contributor.authorLopez-Sanchez, A. R.
dc.contributor.authorMao, M. Y.
dc.contributor.authorMurphy, T.
dc.contributor.authorMessias, H.
dc.contributor.authorPimbblet, K. A.
dc.contributor.authorRaccanelli, A.
dc.contributor.authorRandall, K. E.
dc.contributor.authorReiprich, T. H.
dc.contributor.authorRoseboom, I. G.
dc.contributor.authorRoettgering, H.
dc.contributor.authorSaikia, D. J.
dc.contributor.authorSharp, R. G.
dc.contributor.authorSlee, O. B.
dc.contributor.authorSmail, Ian
dc.contributor.authorThompson, Mark
dc.contributor.authorUrquhart, J. S.
dc.contributor.authorWall, J. V.
dc.contributor.authorZhao, G. -B.
dc.date.accessioned2011-10-24T09:01:15Z
dc.date.available2011-10-24T09:01:15Z
dc.date.issued2011
dc.identifier.citationNorris , R P , Hopkins , A M , Afonso , J , Brown , S , Condon , J J , Dunne , L , Feain , I , Hollow , R , Jarvis , M J , Johnston-Hollitt , M , Lenc , E , Middelberg , E , Padovani , P , Prandoni , I , Rudnick , L , Seymour , N , Umana , G , Andernach , H , Alexander , D M , Appleton , P N , Bacon , D , Banfield , J , Becker , W , Brown , M J I , Ciliegi , P , Jackson , C , Eales , S , Edge , A C , Gaensler , B M , Giovannini , G , Hales , C A , Hancock , P , Huynh , M T , Ibar , E , Ivison , R J , Kennicutt , R , Kimball , A E , Koekemoer , A M , Koribalski , B S , Lopez-Sanchez , A R , Mao , M Y , Murphy , T , Messias , H , Pimbblet , K A , Raccanelli , A , Randall , K E , Reiprich , T H , Roseboom , I G , Roettgering , H , Saikia , D J , Sharp , R G , Slee , O B , Smail , I , Thompson , M , Urquhart , J S , Wall , J V & Zhao , G -B 2011 , ' EMU : Evolutionary Map of the Universe ' , Publications of the Astronomical Society of Australia , vol. 28 , no. 3 , pp. 215-248 . https://doi.org/10.1071/AS11021
dc.identifier.issn1323-3580
dc.identifier.otherPURE: 428589
dc.identifier.otherPURE UUID: 124cd285-9d73-4d83-81dc-ab8d7e33c67a
dc.identifier.otherWOS: 000295162500003
dc.identifier.otherArXiv: http://arxiv.org/abs/1106.3219v1
dc.identifier.otherScopus: 80053408029
dc.identifier.otherORCID: /0000-0001-5392-909X/work/30970830
dc.identifier.urihttp://hdl.handle.net/2299/6766
dc.descriptionOriginal article can be found at: http://www.publish.csiro.au/ Copyright CSIRO Publishing
dc.description.abstractEMU is a wide-field radio continuum survey planned for the new Australian Square Kilometre Array Pathfinder (ASKAP) telescope. The primary goal of EMU is to make a deep (rms ~ 10 microJy/beam) radio continuum survey of the entire Southern Sky at 1.3 GHz, extending as far North as +30 degrees declination, with a resolution of 10 arcsec. EMU is expected to detect and catalogue about 70 million galaxies, including typical star-forming galaxies up to z~1, powerful starbursts to even greater redshifts, and AGNs to the edge of the visible Universe. It will undoubtedly discover new classes of object. This paper defines the science goals and parameters of the survey, and describes the development of techniques necessary to maximise the science return from EMU.en
dc.format.extent34
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of Australia
dc.rightsOpen
dc.subjecttelescopes
dc.subjectsurveys
dc.subjectstars: activity
dc.subjectgalaxies: evolution
dc.subjectgalaxies: formation
dc.subjectcosmology: observations
dc.subjectradio continuum: general
dc.titleEMU : Evolutionary Map of the Universeen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2011
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1071/AS11021
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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