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dc.contributor.authorDavies, L.J.M.
dc.contributor.authorDriver, S.P.
dc.contributor.authorRobotham, A.S.G.
dc.contributor.authorBaldry, I.K.
dc.contributor.authorLange, R.
dc.contributor.authorLiske, J.
dc.contributor.authorMeyer, M.
dc.contributor.authorPopping, A.
dc.contributor.authorWilkins, S.M.
dc.contributor.authorWright, A.H.
dc.date.accessioned2015-03-03T13:01:09Z
dc.date.available2015-03-03T13:01:09Z
dc.date.issued2015-02-11
dc.identifier.citationDavies , L J M , Driver , S P , Robotham , A S G , Baldry , I K , Lange , R , Liske , J , Meyer , M , Popping , A , Wilkins , S M & Wright , A H 2015 , ' Galaxy And Mass Assembly (GAMA) : curation and reanalysis of 16.6k redshifts in the G10/COSMOS region ' Monthly Notices of the Royal Astronomical Society , vol. 447 , no. 1 , pp. 1014-1027 . DOI: 10.1093/mnras/stu2515en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 172285831
dc.identifier.otherPURE UUID: 51eac175-4512-4a61-8109-5b683b1a6f72
dc.identifier.otherScopus: 84922452447
dc.identifier.urihttp://hdl.handle.net/10023/6162
dc.description.abstractWe discuss the construction of the Galaxy And Mass Assembly (GAMA) 10h region (G10) using publicly available data in the Cosmic Evolution Survey region (COSMOS) in order to extend the GAMA survey to z ∼ 1 in a single deg2 field. In order to obtain the maximum number of high precision spectroscopic redshifts we re-reduce all archival zCOSMOS-bright data and use the GAMA automatic cross-correlation redshift fitting code autoz. We use all available redshift information (autoz, zCOSMOS-bright 10k, PRIMUS, VVDS, SDSS and photometric redshifts) to calculate robust best-fitting redshifts for all galaxies and visually inspect all 1D and 2D spectra to obtain 16 583 robust redshifts in the full COSMOS region. We then define the G10 region to be the central ∼1 deg2 of COSMOS, which has relatively high spectroscopic completeness, and encompasses the CHILES VLA region. We define a combined r < 23.0 mag and i < 22.0 mag G10 sample (selected to have the highest bijective overlap) with which to perform future analysis, containing 9861 sources with reliable high-precision VLT-VIMOS spectra. All tables, spectra and imaging are available at http://ict.icrar.org/cutout/G10.en
dc.format.extent14en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rightsThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Societyen
dc.subjectCataloguesen
dc.subjectSurveysen
dc.subjectGalaxies: distances and redshiftsen
dc.subjectGalxies: generalen
dc.subjectGalaxies: high-redshiften
dc.subjectQC Physicsen
dc.subjectDASen
dc.subject.lccQCen
dc.titleGalaxy And Mass Assembly (GAMA) : curation and reanalysis of 16.6k redshifts in the G10/COSMOS regionen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnras/stu2515
dc.description.statusPeer revieweden


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