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dc.contributor.authorLodieu, N.
dc.contributor.authorPinfield, D.J.
dc.contributor.authorLeggett, S.K.
dc.contributor.authorJameson, R.F.
dc.contributor.authorMortlock, D.J.
dc.contributor.authorWarren, S.J.
dc.contributor.authorBurningham, B.
dc.contributor.authorLucas, P.W.
dc.contributor.authorChiu, K.
dc.contributor.authorLiu, M.C.
dc.contributor.authorVenemans, B.P.
dc.contributor.authorMcMahon, R.G.
dc.contributor.authorAllard, F.
dc.contributor.authorBaraffe, I.
dc.contributor.authorNavascue, D.B.Y.
dc.contributor.authorCarraro, G.
dc.contributor.authorCasewell, S.L.
dc.contributor.authorChabrier, G.
dc.contributor.authorChappelle, R.J.
dc.contributor.authorClarke, F.
dc.contributor.authorDay-Jones, A.C.
dc.contributor.authorDeacon, N.R.
dc.contributor.authorDobbie, P.D.
dc.contributor.authorFolkes, S.L.
dc.contributor.authorHambly, N.C.
dc.contributor.authorHewett, P.C.
dc.contributor.authorHodgkin, S.T.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorKendall, T.R.
dc.contributor.authorMagazzu, A.
dc.contributor.authorMartin, E.L.
dc.contributor.authorMcCaughrean, M.J.
dc.contributor.authorNakajima, T.
dc.contributor.authorPavlenko, Y.
dc.contributor.authorTamura, M.
dc.contributor.authorTinney, C.G.
dc.contributor.authorOsorio, M.R.Z.
dc.date.accessioned2015-04-14T12:47:59Z
dc.date.issued2007-07-26
dc.description.abstractWe present eight new T4.5-T7.5 dwarfs identified in the UKIRT (United Kingdom Infrared Telescope) Infrared Deep Sky Survey (UKIDSS) Large Area Survey (LAS) Data Release 1 (DR1). In addition we have recovered the T4.5 dwarf SDSS J020742.91+000056.2 and the T8.5 dwarf ULAS J003402.77-005206.7. Photometric candidates were picked up in two-colour diagrams over 190 deg(2) (DR1) and selected in at least two filters. All candidates exhibit near-infrared spectra with strong methane and water absorption bands characteristic of T dwarfs and the derived spectral types follow the unified scheme of Burgasser et al.. We have found six new T4.5-T5.5 dwarfs, one T7 dwarf, one T7.5 dwarf and recovered a T4.5 dwarf and a T8.5 dwarf. We provide distance estimates which lie in the 15-85 pc range; the T7.5 and T8.5 dwarfs are probably within 25 pc of the Sun. We conclude with a discussion of the number of T dwarfs expected after completion of the LAS, comparing these initial results to theoretical simulations.en_GB
dc.description.sponsorshipNSFen_GB
dc.description.sponsorshipAlfred P. Sloan Research Fellowshipen_GB
dc.identifier.citationVol. 379 (4), pp. 1423 - 1430en_GB
dc.identifier.doi10.1111/j.1365-2966.2007.12023.x
dc.identifier.grantnumberAST-0407441en_GB
dc.identifier.grantnumberAST-0507833en_GB
dc.identifier.urihttp://hdl.handle.net/10871/16799
dc.language.isoenen_GB
dc.publisherOxford University Press for Royal Astronomical Societyen_GB
dc.subjecttechniques : photometricen_GB
dc.subjecttechniques : spectroscopicen_GB
dc.subjectsurveysen_GB
dc.subjectstars : low-massen_GB
dc.subjectbrown dwarfsen_GB
dc.subjectinfrared : starsen_GB
dc.subjectdeep sky surveyen_GB
dc.subjectspectral type-Len_GB
dc.subjectT-dwarfsen_GB
dc.subjectbrown dwarfen_GB
dc.subjectultracool dwarfsen_GB
dc.subjectinfrared photometryen_GB
dc.subjectadaptive opticsen_GB
dc.subjectL/T transitionen_GB
dc.subjectmass functionen_GB
dc.subjecttelescopeen_GB
dc.titleEight new T4.5-T7.5 dwarfs discovered in the UKIDSS large area survey data release 1en_GB
dc.typeArticleen_GB
dc.date.available2015-04-14T12:47:59Z
dc.identifier.issn0035-8711
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2007 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


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