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dc.contributor.authorVerbeek, Kars
dc.contributor.authorde Groot, Eelco
dc.contributor.authorGroot, Paul J.
dc.contributor.authorScaringi, Simone
dc.contributor.authorDrew, J.E.
dc.contributor.authorGreimel, Robert
dc.contributor.authorIrwin, Mike
dc.contributor.authorGonzalez-Solares, Eduardo
dc.contributor.authorGaensicke, Boris T.
dc.contributor.authorCasares, Jorge
dc.contributor.authorCorral-Santana, Jesus M.
dc.contributor.authorDeacon, Niall
dc.contributor.authorSteeghs, Danny
dc.date.accessioned2012-03-12T10:59:59Z
dc.date.available2012-03-12T10:59:59Z
dc.date.issued2012-02
dc.identifier.citationVerbeek , K , de Groot , E , Groot , P J , Scaringi , S , Drew , J E , Greimel , R , Irwin , M , Gonzalez-Solares , E , Gaensicke , B T , Casares , J , Corral-Santana , J M , Deacon , N & Steeghs , D 2012 , ' A first catalogue of automatically selected ultraviolet-excess sources from the UVEX survey ' , Monthly Notices of the Royal Astronomical Society , vol. 420 , no. 2 , pp. 1115-1134 . https://doi.org/10.1111/j.1365-2966.2011.20094.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 622150
dc.identifier.otherPURE UUID: 71cb88df-83de-44af-a0dc-ccffb76a09a0
dc.identifier.otherWOS: 000299417600014
dc.identifier.otherScopus: 84856209242
dc.identifier.urihttp://hdl.handle.net/2299/7932
dc.description.abstractWe present the first catalogue of point-source ultraviolet (UV)-excess sources selected from the UV-Excess Survey of the Northern Galactic Plane (UVEX). UVEX images the Northern Galactic Plane in the U, g, r and He Iota lambda 5875 bands in the Galactic latitude range -5 degrees < b < +5 degrees. Through an automated algorithm, which works on a field-to-field basis, we select blue UV-excess sources in 211 square degrees from the (U-g) versus (g-r) colour-colour diagram and the g versus (U-g) and g versus (g-r) colour-magnitude diagrams. The UV-excess catalogue covers the magnitude range 14 < g < 22.5, contains 2170 sources and consists of a mix of white dwarfs, post-common-envelope objects, interacting binaries, quasars and active galactic nuclei. Two other samples of outliers were found during the selection: (i) a subdwarf sample, consisting of no less than 9872 candidate metal-poor stars or lightly reddened main-sequence stars, and (ii) a purple sample consisting of 803 objects, most likely a mix of reddened late M giants, T Tauri stars, planetary nebulae, symbiotic stars and carbon stars. Cross-matching the selected UV-excess catalogue with other catalogues aids with the first classification of the different populations and shows that more than 99 per cent of our selected sources are unidentified sources.en
dc.format.extent20
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectsurveys
dc.subjectstars: general
dc.subjectISM: general
dc.subjectGalaxy: disc
dc.subjectGalaxy: stellar content
dc.subjectGalaxy: structure
dc.subjectNORTHERN GALACTIC PLANE
dc.subjectH-ALPHA SURVEY
dc.subjectSYMBIOTIC STARS
dc.subjectIPHAS
dc.subjectPOPULATION
dc.subjectEMISSION
dc.subjectNEBULAE
dc.titleA first catalogue of automatically selected ultraviolet-excess sources from the UVEX surveyen
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.date.embargoedUntil2012-08-01
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2011.20094.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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