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WASP-120 b, WASP-122 b, AND WASP-123 b : three newly discovered planets from the WASP-South survey

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dc.contributor.authorTurner, O. D.
dc.contributor.authorAnderson, D. R.
dc.contributor.authorCameron, Andrew Collier
dc.contributor.authorDelrez, L.
dc.contributor.authorEvans, D. F.
dc.contributor.authorGillon, M.
dc.contributor.authorHellier, C.
dc.contributor.authorJehin, E.
dc.contributor.authorLendl, M.
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.authorSmith, A. M. S.
dc.contributor.authorTriaud, A. H. M. J.
dc.contributor.authorUdry, S.
dc.contributor.authorWest, R. G.
dc.date.accessioned2017-05-17T23:33:46Z
dc.date.available2017-05-17T23:33:46Z
dc.date.issued2016-06
dc.identifier.citationTurner , O D , Anderson , D R , Cameron , A C , Delrez , L , Evans , D F , Gillon , M , Hellier , C , Jehin , E , Lendl , M , Maxted , P F L , Pepe , F , Pollacco , D , Queloz , D , Ségransan , D , Smalley , B , Smith , A M S , Triaud , A H M J , Udry , S & West , R G 2016 , ' WASP-120 b, WASP-122 b, AND WASP-123 b : three newly discovered planets from the WASP-South survey ' , Publications of the Astronomical Society of the Pacific , vol. 128 , no. 964 , 64401 . https://doi.org/10.1088/1538-3873/128/964/064401en
dc.identifier.issn0004-6280
dc.identifier.otherPURE: 243086721
dc.identifier.otherPURE UUID: 3a545240-be34-4d45-b1ea-f222584a2dad
dc.identifier.otherBibCode: 2016PASP..128f4401T
dc.identifier.otherScopus: 84973515274
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531390
dc.identifier.otherWOS: 000387110500004
dc.identifier.urihttp://hdl.handle.net/10023/10795
dc.description.abstractWe present the discovery by the WASP-South survey of three planets transiting moderately bright stars (V ≈ 11). WASP-120 b is a massive (4.85 M Jup) planet in a 3.6-day orbit that we find likely to be eccentric (e={0.059}-0.018+0.025) around an F5 star. WASP-122 b is a hot Jupiter (1.28 M Jup, 1.74 R Jup) in a 1.7-day orbit about a G4 star. Our predicted transit depth variation caused by the atmosphere of WASP-122 b suggests it is well suited to characterization. WASP-123 b is a hot Jupiter (0.90M Jup, 1.32 R Jup) in a 3.0-day orbit around an old (∼7 Gyr) G5 star.
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of the Pacificen
dc.rights© 2016, Astronomical Society of the Pacific. This work is made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at iopscience.iop.org / https://dx.doi.org/10.1088/1538-3873/128/964/064401en
dc.subjectPlanetary systemsen
dc.subjectStars: individual (WASP-120, WASP-122, WASP-123)en
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleWASP-120 b, WASP-122 b, AND WASP-123 b : three newly discovered planets from the WASP-South surveyen
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1088/1538-3873/128/964/064401
dc.description.statusPeer revieweden
dc.date.embargoedUntil2017-05-17
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2016PASP..128f4401Ten
dc.identifier.grantnumberST/M001296/1en


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