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dc.contributor.authorBarkaoui, K.
dc.contributor.authorBurdanov, A.
dc.contributor.authorHellier, C.
dc.contributor.authorGillon, M.
dc.contributor.authorSmalley, B.
dc.contributor.authorMaxted, P. F. L.
dc.contributor.authorLendl, M.
dc.contributor.authorTriaud, A. H. M. J.
dc.contributor.authorAnderson, J.
dc.contributor.authorMcCormac, J.
dc.contributor.authorJehin, E.
dc.contributor.authorAlmleaky, Y.
dc.contributor.authorArmstrong, D. J.
dc.contributor.authorBenkhaldoun, Z.
dc.contributor.authorBouchy, F.
dc.contributor.authorBrown, D. J. A.
dc.contributor.authorCameron, A. C.
dc.contributor.authorDaassou, A.
dc.contributor.authorDelrez, L.
dc.contributor.authorDucrot, E.
dc.contributor.authorFoxell, E.
dc.contributor.authorMurray, C.
dc.contributor.authorNielsen, L. D.
dc.contributor.authorPepe, F.
dc.contributor.authorPollacco, D.
dc.contributor.authorPozuelos, F. J.
dc.contributor.authorQueloz, D.
dc.contributor.authorSegransan, D.
dc.contributor.authorUdry, S.
dc.contributor.authorThompson, S.
dc.contributor.authorWest, R. G.
dc.date.accessioned2018-11-30T10:30:14Z
dc.date.available2018-11-30T10:30:14Z
dc.date.issued2019-02
dc.identifier.citationBarkaoui , K , Burdanov , A , Hellier , C , Gillon , M , Smalley , B , Maxted , P F L , Lendl , M , Triaud , A H M J , Anderson , J , McCormac , J , Jehin , E , Almleaky , Y , Armstrong , D J , Benkhaldoun , Z , Bouchy , F , Brown , D J A , Cameron , A C , Daassou , A , Delrez , L , Ducrot , E , Foxell , E , Murray , C , Nielsen , L D , Pepe , F , Pollacco , D , Pozuelos , F J , Queloz , D , Segransan , D , Udry , S , Thompson , S & West , R G 2019 , ' Discovery of three new transiting hot Jupiters: WASP-161 b, WASP-163 b and WASP-170 b ' , Astronomical Journal , vol. 157 , no. 2 , 43 . https://doi.org/10.3847/1538-3881/aaf422en
dc.identifier.issn0004-6256
dc.identifier.otherPURE: 256707295
dc.identifier.otherPURE UUID: e423d072-87ab-46f6-921d-09f248fca691
dc.identifier.otherBibCode: 2018arXiv180706548B
dc.identifier.otherScopus: 85062911276
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531501
dc.identifier.otherWOS: 000455842200002
dc.identifier.urihttp://hdl.handle.net/10023/16587
dc.description.abstractWe present the discovery of three new transiting hot Jupiters by the WASP-South project, WASP-161 b, WASP-163 b and WASP-170 b. Follow-up radial velocities obtained with the Euler/CORALIE spectrograph and transit light curves obtained with the TRAPPIST-North, TRAPPIST-South, SPECULOOS-South, NITES, and Euler telescopes have enabled us to determine the masses and radii for these transiting exoplanets. WASP-161 b completes an orbit around its V=11.1 F6V-type host star in 5.406 days, and has a mass M p = 2.5 ± 0.2 MJup and radius R p = 1.14 ± 0.06 RJup. WASP-163 b orbits around its host star (spectral type G8V and magnitude V = 12.5) every 1.609 days, has a mass of M p = 1.9 ± 0.2 MJup and a radius of R p = 1.2 ± 0.1 RJup. WASP-170 b has a mass of 1.7 ± 0.2 MJup and a radius of 1.14 ± 0.09 RJup and is on a 2.344 days orbit around a G1V-type star of magnitude V=12.8. Given the irradiations (~ 109 erg s-1.cm-2) and masses, the three new planets' sizes are in good agreement with classical models of irradiated giant planets.
dc.format.extent10
dc.language.isoeng
dc.relation.ispartofAstronomical Journalen
dc.rights© 2018, American Astronomical Society. 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 as such may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.3847/1538-3881/aaf422en
dc.subjectPlanetary systemsen
dc.subjectTechniques: photometricen
dc.subjectTechniques: radial velocitiesen
dc.subjectTechniques: spectroscopicen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-NDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleDiscovery of three new transiting hot Jupiters: WASP-161 b, WASP-163 b and WASP-170 ben
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/10.3847/1538-3881/aaf422
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2018arXiv180706548Ben


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