J/A+A/594/A50ivo://CDS.VizieR/J/A+A/594/A50doi:10.26093/cds/vizier.35940050CDSLillo-Box J.Demangeon O.Santerne A.Barros S.C.C.Barrado D.,Hebrard G.Osborn H.P.Armstrong D.J.Almenara J.-M.Boisse I.,Bouchy F.Brown D.J.A.Courcol B.Deleuil M.Delgado Mena E.,Diaz R.F.Kirk J.Lam K.W.F.McCormac J.Pollacco D.Rajpurohit A.,Rey J.Santos N.C.Sousa S.G.Tsantaki M.Wilson P.A.2017-06-01T08:52:39Z2016-10-10T08:28:45ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frmultiple-starssolar-system-planetsWe report the discovery of the two hot Jupiters K2-30 b and K2-34 b. The two planets were detected during campaigns 4 and 5 of the extension of the Kepler mission, K2; they transit their main-sequence stars with periods of ~4.099 and ~2.996 days. Subsequent ground-based radial velocity follow-up with SOPHIE, HARPS-N, and CAFE established the planetary nature of the transiting objects. We analyzed the transit signal, radial velocity, and spectral energy distributions of the two systems to characterize their properties. Both planets (K2-30 b and K2-34 b) are bloated hot Jupiters (1.20R_Jup_ and 1.22R_Jup_) around relatively bright (V=13.5 and V=11.5) slow rotating main-sequence (G8 and F9) stars. Thus, these systems are good candidates for detecting the Rossiter-MacLaughlin effect in order to measure their obliquity and for atmospheric studies.2016A&A...594A..50Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/594/A50CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/594/A50https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/594/A50http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/594/A50https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/594/A50https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/594/A50http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/594/A50GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/594/A50/table2Detrended photometric K2 light curve of K2-34recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBJDBarycentric Julian Date (BJD-2400000)dtime.epochdoubleNFluxNormalized fluxphot.flux;arith.ratiodoublee_NFluxrms uncertainty of NFluxstat.errordoubleJ/A+A/594/A50/table1Detrended photometric K2 light curve of K2-30recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBJDBarycentric Julian Date (BJD-2400000)dtime.epochdoubleNFluxNormalized fluxphot.flux;arith.ratiodoublee_NFluxrms uncertainty of NFluxstat.errordouble