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dc.contributor.authorBaldry, I. K.
dc.contributor.authorLiske, J.
dc.contributor.authorBrown, M. J. I.
dc.contributor.authorRobotham, A. S. G.
dc.contributor.authorDriver, S. P.
dc.contributor.authorDunne, L.
dc.contributor.authorAlpaslan, M.
dc.contributor.authorBrough, S.
dc.contributor.authorCluver, M. E.
dc.contributor.authorEardley, E.
dc.contributor.authorFarrow, D. J.
dc.contributor.authorHeymans, C.
dc.contributor.authorHildebrandt, H.
dc.contributor.authorHopkins, A. M.
dc.contributor.authorKelvin, L. S.
dc.contributor.authorLoveday, J.
dc.contributor.authorMoffett, A. J.
dc.contributor.authorNorberg, P.
dc.contributor.authorOwers, M. S.
dc.contributor.authorTaylor, E. N.
dc.contributor.authorWright, A. H.
dc.contributor.authorBamford, S. P.
dc.contributor.authorBland-Hawthorn, J.
dc.contributor.authorBourne, N.
dc.contributor.authorBremer, M. N.
dc.contributor.authorColless, M.
dc.contributor.authorConselice, C. J.
dc.contributor.authorCroom, S. M.
dc.contributor.authorDavies, L. J. M.
dc.contributor.authorFoster, C.
dc.contributor.authorGrootes, M. W.
dc.contributor.authorHolwerda, B. W.
dc.contributor.authorJones, D. H.
dc.contributor.authorKafle, P. R.
dc.contributor.authorKuijken, K.
dc.contributor.authorLara-Lopez, M. A.
dc.contributor.authorLópez-Sánchez , Á. R.
dc.contributor.authorMeyer, M. J.
dc.contributor.authorPhillipps, S.
dc.contributor.authorSutherland, W. J.
dc.contributor.authorKampen, E. van
dc.contributor.authorWilkins, S. M.
dc.date.accessioned2018-01-19T12:30:06Z
dc.date.available2018-01-19T12:30:06Z
dc.date.issued2018-03
dc.identifier.citationBaldry , I K , Liske , J , Brown , M J I , Robotham , A S G , Driver , S P , Dunne , L , Alpaslan , M , Brough , S , Cluver , M E , Eardley , E , Farrow , D J , Heymans , C , Hildebrandt , H , Hopkins , A M , Kelvin , L S , Loveday , J , Moffett , A J , Norberg , P , Owers , M S , Taylor , E N , Wright , A H , Bamford , S P , Bland-Hawthorn , J , Bourne , N , Bremer , M N , Colless , M , Conselice , C J , Croom , S M , Davies , L J M , Foster , C , Grootes , M W , Holwerda , B W , Jones , D H , Kafle , P R , Kuijken , K , Lara-Lopez , M A , López-Sánchez , Á R , Meyer , M J , Phillipps , S , Sutherland , W J , Kampen , E V & Wilkins , S M 2018 , ' Galaxy And Mass Assembly (GAMA) : the G02 field, Herschel-ATLAS target selection and Data Release 3 ' , Monthly Notices of the Royal Astronomical Society , vol. 474 , no. 3 , pp. 2875-3888 . https://doi.org/10.1093/mnras/stx3042en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 252090945
dc.identifier.otherPURE UUID: b88beb2f-0c49-4521-bd0e-d6e885a3f487
dc.identifier.otherArXiv: http://arxiv.org/abs/1711.09139v1
dc.identifier.otherScopus: 85040232156
dc.identifier.otherWOS: 000424347900079
dc.identifier.urihttps://hdl.handle.net/10023/12522
dc.description.abstractWe describe data release 3 (DR3) of the Galaxy And Mass Assembly (GAMA) survey. The GAMA survey is a spectroscopic redshift and multiwavelength photometric survey in three equatorial regions each of 60.0 deg2 (G09, G12, and G15), and two southern regions of 55.7 deg2 (G02) and 50.6 deg2 (G23). DR3 consists of: the first release of data covering the G02 region and of data on H-ATLAS (Herschel – Astrophysical Terahertz Large Area Survey) sources in the equatorial regions; and updates to data on sources released in DR2. DR3 includes 154 809 sources with secure redshifts across four regions. A subset of the G02 region is 95.5 per cent redshift complete to r < 19.8 mag over an area of 19.5 deg2, with 20 086 galaxy redshifts, that overlaps substantially with the XXL survey (X-ray) and VIPERS (redshift survey). In the equatorial regions, the main survey has even higher completeness (98.5 per cent), and spectra for about 75 per cent of H-ATLAS filler targets were also obtained. This filler sample extends spectroscopic redshifts, for probable optical counterparts to H-ATLAS submillimetre sources, to 0.8 mag deeper (r < 20.6 mag) than the GAMA main survey. There are 25 814 galaxy redshifts for H-ATLAS sources from the GAMA main or filler surveys. GAMA DR3 is available at the survey website (www.gama-survey.org/dr3/).
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2017, the Author(s). This work has been made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at https://doi.org/10.1093/mnras/stx3042en
dc.subjectCataloguesen
dc.subjectSurveysen
dc.subjectGalaxies: distances and redshiftsen
dc.subjectGalaxies: photometryen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleGalaxy And Mass Assembly (GAMA) : the G02 field, Herschel-ATLAS target selection and Data Release 3en
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/stx3042
dc.description.statusPeer revieweden


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