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WASP-157b, a transiting hot jupiter observed with K2

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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.identifier249376651
dc.identifier117ce705-4a10-466e-9d0a-6f355d26ca3d
dc.identifier84994525486
dc.identifier000390336400009
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.otherORCID: /0000-0002-8863-7828/work/58531431
dc.identifier.urihttps://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.format.extent574037
dc.language.isoeng
dc.relation.ispartofPublications of the Astronomical Society of the Pacificen
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.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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