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dc.contributor.authorHolwerda, B. W.
dc.contributor.authorBaldry, I. K.
dc.contributor.authorAlpaslan, M.
dc.contributor.authorBauer, A.
dc.contributor.authorBland-Hawthorn, J.
dc.contributor.authorBrough, S.
dc.contributor.authorBrown, M. J. I.
dc.contributor.authorCluver, M. E.
dc.contributor.authorConselice, C.
dc.contributor.authorDriver, S. P.
dc.contributor.authorHopkins, A. M.
dc.contributor.authorJones, D. H.
dc.contributor.authorLópez-Sánchez, Á. R.
dc.contributor.authorLoveday, J.
dc.contributor.authorMeyer, M. J.
dc.contributor.authorMoffett, A.
dc.date.accessioned2018-01-23T11:30:21Z
dc.date.available2018-01-23T11:30:21Z
dc.date.issued2015-06-01
dc.identifier.citationHolwerda , B W , Baldry , I K , Alpaslan , M , Bauer , A , Bland-Hawthorn , J , Brough , S , Brown , M J I , Cluver , M E , Conselice , C , Driver , S P , Hopkins , A M , Jones , D H , López-Sánchez , Á R , Loveday , J , Meyer , M J & Moffett , A 2015 , ' Galaxy And Mass Assembly (GAMA) blended spectra catalog : strong galaxy-galaxy lens and occulting galaxy pair candidates ' , Monthly Notices of the Royal Astronomical Society , vol. 449 , no. 4 , pp. 4277-4287 . https://doi.org/10.1093/mnras/stv589en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 252100148
dc.identifier.otherPURE UUID: bd40e117-683e-4d9f-a3a5-aba1d9f35c61
dc.identifier.otherArXiv: http://arxiv.org/abs/1503.04813v2
dc.identifier.otherScopus: 84930036619
dc.identifier.otherWOS: 000355342000069
dc.identifier.urihttp://hdl.handle.net/10023/12582
dc.description.abstractWe present the catalogue of blended galaxy spectra from the Galaxy And Mass Assembly (GAMA) survey. These are cases where light from two galaxies are significantly detected in a single GAMA fibre. Galaxy pairs identified from their blended spectrum fall into two principal classes: they are either strong lenses, a passive galaxy lensing an emission-line galaxy; or occulting galaxies, serendipitous overlaps of two galaxies, of any type. Blended spectra can thus be used to reliably identify strong lenses for follow-up observations (high-resolution imaging) and occulting pairs, especially those that are a late-type partly obscuring an early-type galaxy which are of interest for the study of dust content of spiral and irregular galaxies. The GAMA survey setup and its autoz automated redshift determination were used to identify candidate blended galaxy spectra from the cross-correlation peaks. We identify 280 blended spectra with a minimum velocity separation of 600 km s−1, of which 104 are lens pair candidates, 71 emission-line-passive pairs, 78 are pairs of emission-line galaxies and 27 are pairs of galaxies with passive spectra. We have visually inspected the candidates in the Sloan Digital Sky Survey (SDSS) and Kilo Degree Survey (KiDS) images. Many blended objects are ellipticals with blue fuzz (Ef in our classification). These latter ‘Ef’ classifications are candidates for possible strong lenses, massive ellipticals with an emission-line galaxy in one or more lensed images. The GAMA lens and occulting galaxy candidate samples are similar in size to those identified in the entire SDSS. This blended spectrum sample stands as a testament of the power of this highly complete, second-largest spectroscopic survey in existence and offers the possibility to expand e.g. strong gravitational lens surveys.
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2015, 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/stv589en
dc.subjectGravitational lensing: strongen
dc.subjectCataloguesen
dc.subjectDusten
dc.subjectExtinctionen
dc.subjectGalaxies: distances and redshiftsen
dc.subjectGalaxies: statisticsen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleGalaxy And Mass Assembly (GAMA) blended spectra catalog : strong galaxy-galaxy lens and occulting galaxy pair candidatesen
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/stv589
dc.description.statusPeer revieweden


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