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dc.contributor.authorDeacon, Niall
dc.contributor.authorGroot, P.
dc.contributor.authorDrew, J.E.
dc.contributor.authorGreimel, R.
dc.contributor.authorHambly, N.C.
dc.contributor.authorIrwin, M.J.
dc.contributor.authorAungwerojwit, A.
dc.contributor.authorDrake, J.
dc.contributor.authorSteeghs, D.
dc.date.accessioned2009-12-22T11:41:39Z
dc.date.available2009-12-22T11:41:39Z
dc.date.issued2009
dc.identifier.citationDeacon , N , Groot , P , Drew , J E , Greimel , R , Hambly , N C , Irwin , M J , Aungwerojwit , A , Drake , J & Steeghs , D 2009 , ' The IPHAS-POSS-I proper motion survey of the Galactic plane ' , Monthly Notices of the Royal Astronomical Society , vol. 397 , no. 3 , pp. 1685-1694 . https://doi.org/10.1111/j.1365-2966.2009.15077.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 151859
dc.identifier.otherPURE UUID: 0bc40f3d-4c46-477a-88b1-a98ece9a730c
dc.identifier.otherdspace: 2299/4120
dc.identifier.otherScopus: 68149163453
dc.identifier.urihttp://hdl.handle.net/2299/4120
dc.description‘The definitive version is available at www3.interscience.wiley.com '. Copyright Royal Astronomical Society. DOI: 10.1111/j.1365-2966.2009.15077.x
dc.description.abstractWe present a proper motion survey of the Galactic plane, using Isaac Newton Telescope (INT) Photometric Hα Survey (IPHAS) data and Palomar Sky Survey (POSS)-I Schmidt plate data as a first epoch, that probes down to proper motions below 50 mas yr−1. The IPHAS survey covers the northern plane (|b| < 5°) with CCD photometry in the r, i and Hα passbands. We examine roughly 1400 deg2 of the IPHAS survey area and draw up a catalogue containing 103 058 objects with significant proper motions below 150 mas yr−1 in the magnitude range 13.5 < r' < 19 . Our survey sample contains large samples of white dwarfs and subdwarfs which can be identified using a reduced proper motion diagram. We also found several objects with IPHAS colours suggesting Hα emission and significant proper motions. One is the known cataclysmic variable GD552; two are known DB white dwarfs and five others are found to be non-DA (DB and DC) white dwarfs, which were included in the Hα emission line catalogue due to their lack of absorption in the Hα narrow band.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleThe IPHAS-POSS-I proper motion survey of the Galactic planeen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2009.15077.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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