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dc.contributor.authorBurningham, B.
dc.contributor.authorLucas, P.W.
dc.contributor.authorLeggett, S.K.
dc.contributor.authorSmart, R.
dc.contributor.authorBaker, D.
dc.contributor.authorPinfield, D.J.
dc.contributor.authorTinney, C. G.
dc.contributor.authorHomeier, D.
dc.contributor.authorAllard, F.
dc.contributor.authorZhang, Z. H.
dc.contributor.authorGomes, J.
dc.contributor.authorDay-Jones, A. C.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorKovacs, G.
dc.contributor.authorLodieu, N.
dc.contributor.authorMarocco, F.
dc.contributor.authorMurray, D. N.
dc.contributor.authorSipocz, B.
dc.date.accessioned2011-09-15T11:01:20Z
dc.date.available2011-09-15T11:01:20Z
dc.date.issued2011-06
dc.identifier.citationBurningham , B , Lucas , P W , Leggett , S K , Smart , R , Baker , D , Pinfield , D J , Tinney , C G , Homeier , D , Allard , F , Zhang , Z H , Gomes , J , Day-Jones , A C , Jones , H R A , Kovacs , G , Lodieu , N , Marocco , F , Murray , D N & Sipocz , B 2011 , ' The discovery of the T8.5 dwarf UGPS J0521+3640 ' , Monthly Notices of the Royal Astronomical Society , vol. 414 , no. 1 , pp. L90-L94 . https://doi.org/10.1111/j.1745-3933.2011.01062.x
dc.identifier.issn0035-8711
dc.identifier.otherORCID: /0000-0002-8872-4462/work/62748891
dc.identifier.otherORCID: /0000-0003-4600-5627/work/64327339
dc.identifier.urihttp://hdl.handle.net/2299/6446
dc.descriptionThe definitive version can be found at: http://onlinelibrary.wiley.com/ Copyright Royal Astronomical Society
dc.description.abstractWe have carried out a search for late-type T dwarfs in the UKIRT Infrared Deep Sky Survey Galactic Plane Survey 6th Data Release. The search yielded two persuasive candidates, both of which have been confirmed as T dwarfs. The brightest, UGPS J0521+3640, has been assigned the spectral type T8.5 and appears to lie at a distance of 7-9 pc. The fainter of the two, UGPS J0652+0324, is classified as a T5.5 dwarf and lies at an estimated distance of 28-37 pc. Warm-Spitzer observations in IRAC channels 1 and 2, taken as part of the GLIMPSE360 Legacy Survey, are available for UGPS J0521+3640 and we used these data with the near-infrared spectroscopy to estimate its properties. We find best-fitting solar metallicity BT-Settl models for T-eff = 600 and 650 K and log g = 4.5 and 5.0. These parameters suggest a mass between 14 and 32M(J) for an age between 1 and 5 Gyr. The proximity of this very cool T dwarf, and its location in the Galactic plane, makes it an ideal candidate for high-resolution adaptive optics imaging to search for cool companions.en
dc.format.extent5
dc.format.extent345286
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectsurveys
dc.subjectbrown dwarfs
dc.subjectstars: low-mass
dc.titleThe discovery of the T8.5 dwarf UGPS J0521+3640en
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.embargoedUntil2011-11-01
rioxxterms.versionofrecord10.1111/j.1745-3933.2011.01062.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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