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dc.contributor.authorHellier, Coel
dc.contributor.authorTriaud, A. H. M. J.
dc.contributor.authorBouchy, F.
dc.contributor.authorBurdanov, A.
dc.contributor.authorCameron, A. Collier
dc.contributor.authorDelrez, L.
dc.contributor.authorEhrenreich, D.
dc.contributor.authorGillon, M.
dc.contributor.authorJehin, E.
dc.contributor.authorLendl, M.
dc.contributor.authorLinder, E.
dc.contributor.authorNielsen, L. D.
dc.contributor.authorMaxted, P. F. L.
dc.contributor.authorPepe, F.
dc.contributor.authorPollacco, D.
dc.contributor.authorQueloz, D.
dc.contributor.authorSégransan, D.
dc.contributor.authorSmalley, B.
dc.contributor.authorSpake, J. J.
dc.contributor.authorTemple, L. Y.
dc.contributor.authorUdry, S.
dc.contributor.authorWest, R. G.
dc.contributor.authorWyttenbach, A.
dc.date.accessioned2019-07-22T13:30:01Z
dc.date.available2019-07-22T13:30:01Z
dc.date.issued2019-09
dc.identifier260248206
dc.identifierf15715b7-9a45-413f-bb73-f1d73b79cf58
dc.identifier85072405288
dc.identifier000485158400009
dc.identifier.citationHellier , C , Triaud , A H M J , Bouchy , F , Burdanov , A , Cameron , A C , Delrez , L , Ehrenreich , D , Gillon , M , Jehin , E , Lendl , M , Linder , E , Nielsen , L D , Maxted , P F L , Pepe , F , Pollacco , D , Queloz , D , Ségransan , D , Smalley , B , Spake , J J , Temple , L Y , Udry , S , West , R G & Wyttenbach , A 2019 , ' WASP-166b : a bloated super-Neptune transiting a V = 9 star ' , Monthly Notices of the Royal Astronomical Society , vol. 488 , no. 3 , pp. 3067-3075 . https://doi.org/10.1093/mnras/stz1903en
dc.identifier.issn0035-8711
dc.identifier.otherBibCode: 2019MNRAS.tmp.1834H
dc.identifier.otherORCID: /0000-0002-8863-7828/work/59953644
dc.identifier.urihttps://hdl.handle.net/10023/18147
dc.descriptionACC acknowledges support from STFC consolidated grant number ST/R000824/1.en
dc.description.abstractWe report the discovery of WASP-166b, a super-Neptune planet with a mass of 0.1 MJup (1.9 MNep) and a bloated radius of 0.63 RJup. It transits a V = 9.36, F9V star in a 5.44-d orbit that is aligned with the stellar rotation axis (sky-projected obliquity angle λ = 3 ± 5 degrees). Variations in the radial-velocity measurements are likely the result of magnetic activity over a 12-d stellar rotation period. WASP-166b appears to be a rare object within the “Neptune desert”.
dc.format.extent954290
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectPlanetary systemsen
dc.subjectStars: individual (WASP-166)en
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-NDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleWASP-166b : a bloated super-Neptune transiting a V = 9 staren
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.identifier.doi10.1093/mnras/stz1903
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2019MNRAS.tmp.1834Hen
dc.identifier.grantnumberST/R00824/1en


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