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dc.contributor.authorHébrard, G.
dc.contributor.authorCollier Cameron, A.
dc.contributor.authorBrown, D.J.A.
dc.contributor.authorDíaz, R.F.
dc.contributor.authorFaedi, F.
dc.contributor.authorSmalley, B.
dc.contributor.authorAnderson, D.R.
dc.contributor.authorArmstrong, D.
dc.contributor.authorBarros, S.C.C.
dc.contributor.authorBento, J.
dc.contributor.authorBouchy, F.
dc.contributor.authorDoyle, A.P.
dc.contributor.authorEnoch, B.
dc.contributor.authorGómez Maqueo Chew, Y.
dc.contributor.authorHébrard, E.M.
dc.contributor.authorHellier, C.
dc.contributor.authorLendl, M.
dc.contributor.authorLister, T.A.
dc.contributor.authorMaxted, P.F.L.
dc.contributor.authorMcCormac, J.
dc.contributor.authorMoutou, C.
dc.contributor.authorPollacco, D.
dc.contributor.authorQueloz, D.
dc.contributor.authorSanterne, A.
dc.contributor.authorSkillen, I.
dc.contributor.authorSouthworth, J.
dc.contributor.authorTregloan-Reed, J.
dc.contributor.authorTriaud, A.H.M.J.
dc.contributor.authorUdry, S.
dc.contributor.authorVanhuysse, M.
dc.contributor.authorWatson, C.A.
dc.contributor.authorWest, R.G.
dc.contributor.authorWheatley, P.J.
dc.date.accessioned2014-09-23T14:01:03Z
dc.date.available2014-09-23T14:01:03Z
dc.date.issued2013-01
dc.identifier150600370
dc.identifier0f3296e9-331d-4839-8f0d-12bb164a7c4b
dc.identifier84872350393
dc.identifier.citationHébrard , G , Collier Cameron , A , Brown , D J A , Díaz , R F , Faedi , F , Smalley , B , Anderson , D R , Armstrong , D , Barros , S C C , Bento , J , Bouchy , F , Doyle , A P , Enoch , B , Gómez Maqueo Chew , Y , Hébrard , E M , Hellier , C , Lendl , M , Lister , T A , Maxted , P F L , McCormac , J , Moutou , C , Pollacco , D , Queloz , D , Santerne , A , Skillen , I , Southworth , J , Tregloan-Reed , J , Triaud , A H M J , Udry , S , Vanhuysse , M , Watson , C A , West , R G & Wheatley , P J 2013 , ' WASP-52b, WASP-58b, WASP-59b, and WASP-60b : four new transiting close-in giant planets ' , Astronomy & Astrophysics , vol. 549 , A134 . https://doi.org/10.1051/0004-6361/201220363en
dc.identifier.issn0004-6361
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531479
dc.identifier.urihttps://hdl.handle.net/10023/5483
dc.descriptionThe research leading to these results received funding from the European Communitys Seventh Framework Programme (FP7/2007-2013) under grant agreement number RG226604 (OPTICON), as well as the Programme National de Planétologie (PNP) of CNRS/INSU (France).en
dc.description.abstractWe present the discovery of four new transiting hot Jupiters, detected mainly from SuperWASP-North and SOPHIE observations. These new planets, WASP-52b, WASP-58b, WASP-59b, and WASP-60b, have orbital periods ranging from 1.7 to 7.9 days, masses between 0.46 and 0.94 MJup, and radii between 0.73 and 1.49 RJup. Their G1 to K5 dwarf host stars have V magnitudes in the range 11.7−13.0. The depths of the transits are between 0.6 and 2.7%, depending on the target. With their large radii, WASP-52b and WASP-58b are new cases of low-density, inflated planets, whereas WASP-59b is likely to have a large, dense core. WASP-60 shows shallow transits. In the case of WASP-52 we also detected the Rossiter-McLaughlin anomaly via time-resolved spectroscopy of a transit. We measured the sky-projected obliquity λ = 24° +17-9, indicating that WASP-52b orbits in the same direction as its host star is rotating and that this prograde orbit is slightly misaligned with the stellar equator. These four new planetary systems increase our statistics on hot Jupiters and provide new targets for follow-up studies.
dc.format.extent11
dc.format.extent732468
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysicsen
dc.subjectPlanetary systemsen
dc.subjectTechniques: polarimetricen
dc.subjectTechniques: radial velocitiesen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleWASP-52b, WASP-58b, WASP-59b, and WASP-60b : four new transiting close-in giant planetsen
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1051/0004-6361/201220363
dc.description.statusPeer revieweden
dc.identifier.grantnumberST/J001651/1en
dc.identifier.grantnumberPP/F000065/1en


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