Show simple item record

dc.contributor.authorGroot, Paul J.
dc.contributor.authorVerbeek, Kars
dc.contributor.authorGreimel, Robert
dc.contributor.authorIrwin, Mike
dc.contributor.authorGonzález-Solares, Eduardo
dc.contributor.authorGänsicke, Boris T.
dc.contributor.authorde Groot, Eelco
dc.contributor.authorDrew, Janet
dc.contributor.authorAugusteijn, Thomas
dc.contributor.authorAungwerojwit, Amornrat
dc.contributor.authorBarlow, Mike
dc.contributor.authorBarros, Susana
dc.contributor.authorVan Den Besselaar, Else J. M.
dc.contributor.authorCasares, Jorge
dc.contributor.authorCorradi, Romano
dc.contributor.authorCorral-Santana, Jesús M.
dc.contributor.authorDeacon, Niall
dc.contributor.authorvan Ham, Wilbert
dc.contributor.authorHu, Haili
dc.contributor.authorHeber, Uli
dc.contributor.authorJonker, Peter G.
dc.contributor.authorKing, Rob
dc.contributor.authorKnigge, Christian
dc.contributor.authorMampaso, Antonio
dc.contributor.authorMarsh, Tom R.
dc.contributor.authorMorales-Rueda, Luisa
dc.contributor.authorNapiwotzki, Ralf
dc.contributor.authorNaylor, Tim
dc.contributor.authorNelemans, Gijs
dc.contributor.authorOosting, Tim
dc.contributor.authorPyrzas, Stylianos
dc.contributor.authorPretorius, Magaretha
dc.contributor.authorRodríguez-Gil, Pablo
dc.contributor.authorRoelofs, Gijs H. A.
dc.contributor.authorSale, Stuart
dc.contributor.authorSchellart, Pim
dc.contributor.authorSteeghs, Danny
dc.contributor.authorSzyszka, Cezary
dc.contributor.authorUnruh, Yvonne
dc.contributor.authorWalton, Nicholas A.
dc.contributor.authorWeston, Simon
dc.contributor.authorWitham, Andrew
dc.contributor.authorWoudt, Patrick
dc.contributor.authorZijlstra, Albert
dc.date.accessioned2015-05-22T14:25:47Z
dc.date.issued2009
dc.description.abstractThe UV-Excess survey of the northern Galactic plane images a 10° × 185° wide band, centred on the Galactic equator using the 2.5-m Isaac Newton Telescope in four bands (I5875) down to ~21-22 mag ( in I5875). The setup and data reduction procedures are described. Simulations of the colours of main-sequence stars, giant, supergiants, DA and DB white dwarfs and AM Canum Venaticorum stars are made, including the effects of reddening. A first look at the data of the survey (currently 30 per cent complete) is given.en_GB
dc.description.sponsorshipNASAen_GB
dc.description.sponsorshipNSFen_GB
dc.description.sponsorshipNWO-EWen_GB
dc.description.sponsorshipNOVAen_GB
dc.description.sponsorshipNWO-VIDIen_GB
dc.identifier.citationVol. 399 (1), pp. 323 - 339en_GB
dc.identifier.doi10.1111/j.1365-2966.2009.15273.x
dc.identifier.grantnumber614.000.601en_GB
dc.identifier.grantnumber639.042.201en_GB
dc.identifier.urihttp://hdl.handle.net/10871/17280
dc.language.isoenen_GB
dc.publisherOxford University Press for Royal Astronomical Societyen_GB
dc.relation.urlhttp://dx.doi.org/10.1111/j.1365-2966.2009.15273.xen_GB
dc.subjectsurveysen_GB
dc.subjectstars: generalen_GB
dc.subjectISM: generalen_GB
dc.subjectGalaxy: discen_GB
dc.subjectGalaxy: stellar contenten_GB
dc.subjectGalaxy: structureen_GB
dc.titleThe UV-Excess survey of the northern Galactic planeen_GB
dc.typeArticleen_GB
dc.date.available2015-05-22T14:25:47Z
dc.identifier.issn0035-8711
dc.descriptionCopyright © 2009 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.en_GB
dc.identifier.eissn1365-2966
dc.identifier.journalMonthly Notices of the Royal Astronomical Societyen_GB


Files in this item

This item appears in the following Collection(s)

Show simple item record