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dc.contributor.authorCappetta, M.
dc.contributor.authorSaglia, R.P.
dc.contributor.authorBirkby, J. L.
dc.contributor.authorKoppenhoefer, J.
dc.contributor.authorPinfield, D.J.
dc.contributor.authorHodgkin, S.T.
dc.contributor.authorCruz, P.
dc.contributor.authorKovacs, G.
dc.contributor.authorSipocz, B.
dc.contributor.authorBarrado, D.
dc.contributor.authorNefs, B.
dc.contributor.authorPavlenko, Y. V.
dc.contributor.authorFossati, L.
dc.contributor.authorBurgo, C. del
dc.contributor.authorMartin, E. L.
dc.contributor.authorSnellen, I.
dc.contributor.authorBarnes, J.
dc.contributor.authorCampbell, D. A.
dc.contributor.authorCatalan, S.
dc.contributor.authorGalvez-Ortiz, M. C.
dc.contributor.authorGoulding, N.
dc.contributor.authorHaswell, C.
dc.contributor.authorIvanyuk, O.
dc.contributor.authorJones, H.R.A.
dc.contributor.authorKuznetsov, M.
dc.contributor.authorLodieu, N.
dc.contributor.authorMarocco, F.
dc.contributor.authorMislis, D.
dc.contributor.authorMurgas, F.
dc.contributor.authorNapiwotzki, R.
dc.contributor.authorPalle, E.
dc.contributor.authorPollacco, D.
dc.contributor.authorBaro, L. Sarro
dc.contributor.authorSolano, E.
dc.contributor.authorSteele, P.
dc.contributor.authorStoev, H.
dc.contributor.authorTata, R.
dc.contributor.authorZendejas, J.
dc.date.accessioned2015-05-26T15:05:54Z
dc.date.available2015-05-26T15:05:54Z
dc.date.issued2014-11-11
dc.identifier.citationCappetta , M , Saglia , R P , Birkby , J L , Koppenhoefer , J , Pinfield , D J , Hodgkin , S T , Cruz , P , Kovacs , G , Sipocz , B , Barrado , D , Nefs , B , Pavlenko , Y V , Fossati , L , Burgo , C D , Martin , E L , Snellen , I , Barnes , J , Campbell , D A , Catalan , S , Galvez-Ortiz , M C , Goulding , N , Haswell , C , Ivanyuk , O , Jones , H R A , Kuznetsov , M , Lodieu , N , Marocco , F , Mislis , D , Murgas , F , Napiwotzki , R , Palle , E , Pollacco , D , Baro , L S , Solano , E , Steele , P , Stoev , H , Tata , R & Zendejas , J 2014 , ' The first planet detected in the WTS : an inflated hot-Jupiter in a 3.35 day orbit around a late F-star [ERRATUM] ' , Monthly Notices of the Royal Astronomical Society , vol. 444 , no. 4 , stu1662 , pp. 3150 . https://doi.org/10.1093/mnras/stu1662
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 8586049
dc.identifier.otherPURE UUID: fe913d8d-786b-48ea-a70f-135b063e3cc1
dc.identifier.otherArXiv: http://arxiv.org/abs/1410.3235v1
dc.identifier.otherScopus: 84929439446
dc.identifier.urihttp://hdl.handle.net/2299/15932
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society. ©: 2014 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
dc.description.abstractWe report the discovery of WTS-1b, the first extrasolar planet found by the WFCAM Transit Survey, which began observations at the 3.8-m United Kingdom Infrared Telescope (UKIRT) in August 2007. Light curves comprising almost 1200 epochs with a photometric precision of better than 1 per cent to J ~ 16 were constructed for ~60000 stars and searched for periodic transit signals. For one of the most promising transiting candidates, high-resolution spectra taken at the Hobby-Eberly Telescope (HET) allowed us to estimate the spectroscopic parameters of the host star, a late-F main sequence dwarf (V=16.13) with possibly slightly subsolar metallicity, and to measure its radial velocity variations. The combined analysis of the light curves and spectroscopic data resulted in an orbital period of the substellar companion of 3.35 days, a planetary mass of 4.01 +- 0.35 Mj and a planetary radius of 1.49+0.16-0.18 Rj. WTS-1b has one of the largest radius anomalies among the known hot Jupiters in the mass range 3-5 Mj. The high irradiation from the host star ranks the planet in the pM class.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectastro-ph.EP
dc.titleThe first planet detected in the WTS : an inflated hot-Jupiter in a 3.35 day orbit around a late F-star [ERRATUM]en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnras/stu1662
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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