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dc.contributor.authorSmith, Leigh
dc.contributor.authorLucas, P.W.
dc.contributor.authorBurningham, B.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorPinfield, D.J.
dc.contributor.authorSmart, Ricky
dc.contributor.authorAndrei, Alexandre
dc.contributor.editorSaglia, R.
dc.date.accessioned2014-07-16T12:00:10Z
dc.date.available2014-07-16T12:00:10Z
dc.date.issued2013
dc.identifier.citationSmith , L , Lucas , P W , Burningham , B , Jones , H R A , Pinfield , D J , Smart , R & Andrei , A 2013 , A 2 epoch proper motion catalogue from the UKIDSS Large Area Survey . in R Saglia (ed.) , Hot Planets and Cool Stars . , 06006 , EPJ Web of Conferences , vol. 47 , EDP Sciences , Conference on Hot Planets and Cool Stars , Germany , 12/11/12 . https://doi.org/10.1051/epjconf/20134706006
dc.identifier.citationconference
dc.identifier.issn2100-014X
dc.identifier.otherPURE: 7179770
dc.identifier.otherPURE UUID: bc9425f0-c159-4609-a31b-49cf5a1693d6
dc.identifier.otherWOS: 000319988900037
dc.identifier.otherScopus: 84877613589
dc.identifier.otherORCID: /0000-0002-8872-4462/work/62748832
dc.identifier.otherORCID: /0000-0003-4600-5627/work/64327308
dc.identifier.urihttp://hdl.handle.net/2299/13943
dc.descriptionThis is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited
dc.description.abstractThe UKIDSS Large Area Survey (LAS) began in 2005, with the start of the UKIDSS program as a 7 year effort to survey roughly 4000 square degrees at high galactic latitudes in Y, J, H and K bands. The survey also included a significant quantity of 2-epoch J band observations, with epoch baselines ranging from 2 to 7 years. We present a proper motion catalogue for the 1500 square degrees of the 2 epoch LAS data, which includes some 800,000 sources with motions detected above the 5 sigma level. We developed a bespoke proper motion pipeline which applies a source-unique second order polynomial transformation to UKIDSS array coordinates of each source to counter potential local non-uniformity in the focal plane. Our catalogue agrees well with the proper motion data supplied in the current WFCAM Science Archive (WSA) DR9 catalogue where there is overlap, and in various optical catalogues, but it benefits from some improvements. One improvement is that we provide absolute proper motions, using LAS galaxies for the relative to absolute correction. Also, by using unique, local, 2nd order polynomial tranformations, as opposed to the linear transformations in the WSA, we correct better for any local distortions in the focal plane, not including the radial distortion that is removed by their pipeline.en
dc.format.extent3
dc.language.isoeng
dc.publisherEDP Sciences
dc.relation.ispartofHot Planets and Cool Stars
dc.relation.ispartofseriesEPJ Web of Conferences
dc.subjectSTARS
dc.titleA 2 epoch proper motion catalogue from the UKIDSS Large Area Surveyen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1051/epjconf/20134706006
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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