Show simple item record

Files in this item

Thumbnail

Item metadata

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.date.accessioned2014-09-08T13:31:02Z
dc.date.available2014-09-08T13:31:02Z
dc.date.issued2014-05-21
dc.identifier146751493
dc.identifierf850d7ff-c028-467a-aa18-fc0b51bbdb14
dc.identifier000334744000007
dc.identifier84898809480
dc.identifier000334744000007
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 . https://doi.org/10.1093/mnras/stu410en
dc.identifier.issn0035-8711
dc.identifier.otherORCID: /0000-0002-8863-7828/work/58531370
dc.identifier.urihttps://hdl.handle.net/10023/5374
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.format.extent11
dc.format.extent6426738
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectPlanetary systemsen
dc.subjectLight curvesen
dc.subjectB 2en
dc.subjectPlaneten
dc.subjectStarsen
dc.subjectSuperwaspen
dc.subjectEvolutionen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject.lccQBen
dc.subject.lccQCen
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.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1093/mnras/stu410
dc.description.statusPeer revieweden
dc.identifier.urlhttp://mnras.oxfordjournals.org/content/440/3/1982/suppl/DC1en
dc.identifier.grantnumberST/J001651/1en
dc.identifier.grantnumberPP/F000065/1en


This item appears in the following Collection(s)

Show simple item record