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dc.contributor.authorHellier, Coel
dc.contributor.authorAnderson, D. R.
dc.contributor.authorCameron, A. Collier
dc.contributor.authorDelrez, L.
dc.contributor.authorGillon, M.
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.authorSegransan, D.
dc.contributor.authorSmalley, B.
dc.contributor.authorSmith, A. M. S.
dc.contributor.authorSouthworth, J.
dc.contributor.authorTriaud, A. H. M. J.
dc.contributor.authorUdry, S.
dc.contributor.authorWest, R. G.
dc.identifier.citationHellier , C , Anderson , D R , Cameron , A C , Delrez , L , Gillon , M , Jehin , E , Lendl , M , Maxted , P F L , Pepe , F , Pollacco , D , Queloz , D , Segransan , D , Smalley , B , Smith , A M S , Southworth , J , Triaud , A H M J , Udry , S & West , R G 2014 , ' Transiting hot Jupiters from WASP-South, Euler and TRAPPIST : WASP-95b to WASP-101b ' , Monthly Notices of the Royal Astronomical Society , vol. 440 , no. 3 , pp. 1982-1992 .
dc.identifier.otherPURE: 146751493
dc.identifier.otherPURE UUID: f850d7ff-c028-467a-aa18-fc0b51bbdb14
dc.identifier.otherWOS: 000334744000007
dc.identifier.otherScopus: 84898809480
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531370
dc.identifier.otherWOS: 000334744000007
dc.description.abstractWe report the discovery of the transiting exoplanets WASP-95b, WASP-96b, WASP-97b, WASP-98b, WASP-99b, WASP-100b andWASP-101b. All are hot Jupiters with orbital periods in the range 2.1-5.7 d, masses of 0.5-2.8 MJup and radii of 1.1-1.4 RJup. The orbits of all the planets are compatible with zero eccentricity. WASP-99b produces the shallowest transit yet found by WASP-South, at 0.4 per cent. The host stars are of spectral type F2-G8. Five have metallicities of [Fe/H] from -0.03 to +0.23, while WASP-98 has a metallicity of -0.60, exceptionally low for a star with a transiting exoplanet. Five of the host stars are brighter than V = 10.8, which significantly extends the number of bright transiting systems available for follow-up studies. WASP-95 shows a possible rotational modulation at a period of 20.7 d. We discuss the completeness of WASP survey techniques by comparing to the HATnet project.
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Societyen
dc.subjectPlanetary systemsen
dc.subjectLight curvesen
dc.subjectB 2en
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.titleTransiting hot Jupiters from WASP-South, Euler and TRAPPIST : WASP-95b to WASP-101ben
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.description.statusPeer revieweden

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