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dc.contributor.authorMočnik, T.
dc.contributor.authorAnderson, D. R.
dc.contributor.authorBrown, D. J. A.
dc.contributor.authorCameron, A. Collier
dc.contributor.authorDelrez, L.
dc.contributor.authorGillon, M.
dc.contributor.authorHellier, C.
dc.contributor.authorJehin, E.
dc.contributor.authorLendl, M.
dc.contributor.authorMaxted, P. F. L.
dc.contributor.authorNeveu-Vanmalle, M.
dc.contributor.authorPepe, F.
dc.contributor.authorPollacco, D.
dc.contributor.authorQueloz, D.
dc.contributor.authorSégransan, D.
dc.contributor.authorSmalley, B.
dc.contributor.authorSouthworth, J.
dc.contributor.authorTriaud, A. H. M. J.
dc.contributor.authorUdry, S.
dc.contributor.authorWest, R. G.
dc.date.accessioned2017-12-02T00:32:05Z
dc.date.available2017-12-02T00:32:05Z
dc.date.issued2016-12
dc.identifier.citationMočnik , T , Anderson , D R , Brown , D J A , Cameron , A C , Delrez , L , Gillon , M , Hellier , C , Jehin , E , Lendl , M , Maxted , P F L , Neveu-Vanmalle , M , Pepe , F , Pollacco , D , Queloz , D , Ségransan , D , Smalley , B , Southworth , J , Triaud , A H M J , Udry , S & West , R G 2016 , ' WASP-157b, a transiting hot jupiter observed with K2 ' , Publications of the Astronomical Society of the Pacific , vol. 128 , no. 970 , 124403 . https://doi.org/10.1088/1538-3873/128/970/124403en
dc.identifier.issn0004-6280
dc.identifier.otherPURE: 249376651
dc.identifier.otherPURE UUID: 117ce705-4a10-466e-9d0a-6f355d26ca3d
dc.identifier.otherScopus: 84994525486
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531431
dc.identifier.otherWOS: 000390336400009
dc.identifier.urihttp://hdl.handle.net/10023/12233
dc.descriptionWe gratefully acknowledge the financial support from the Science and Technology Facilities Council (STFC), under grants ST/J001384/1, ST/M001040/1 and ST/M50354X/1.en
dc.description.abstractWe announce the discovery of the transiting hot Jupiter WASP-157b in a 3.95-d orbit around a V = 12.9 G2 mainsequence star. This moderately inflated planet has a Saturn-like density, with a mass of 0.57 ± 0.10 MJup and a radius of 1.06 ± 0.05 RJup. We do not detect any rotational or phase curve modulations, nor the secondary eclipse, with conservative semi-amplitude upper limits of 250 and 20 ppm, respectively.
dc.format.extent7
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of the Pacificen
dc.rights© 2016, The Astronomical Society of the Pacific. This work has been 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 https://doi.org/10.1088/1538-3873/128/970/124403en
dc.subjectPlanets and satellites: Detectionen
dc.subjectPlanets and satellites: Individual (WASP-157b)en
dc.subjectStars: Individual (WASP-157)en
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectAstronomy and Astrophysicsen
dc.subjectSpace and Planetary Scienceen
dc.subject3rd-DASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleWASP-157b, a transiting hot jupiter observed with K2en
dc.typeJournal articleen
dc.description.versionPostprinten
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.doihttps://doi.org/10.1088/1538-3873/128/970/124403
dc.description.statusPeer revieweden
dc.identifier.urlhttps://arxiv.org/abs/1603.05638en


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