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Transiting hot Jupiters from WASP-South, Euler and TRAPPIST : WASP-95b to WASP-101b
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dc.contributor.author | Hellier, Coel | |
dc.contributor.author | Anderson, D. R. | |
dc.contributor.author | Cameron, A. Collier | |
dc.contributor.author | Delrez, L. | |
dc.contributor.author | Gillon, M. | |
dc.contributor.author | Jehin, E. | |
dc.contributor.author | Lendl, M. | |
dc.contributor.author | Maxted, P. F. L. | |
dc.contributor.author | Pepe, F. | |
dc.contributor.author | Pollacco, D. | |
dc.contributor.author | Queloz, D. | |
dc.contributor.author | Segransan, D. | |
dc.contributor.author | Smalley, B. | |
dc.contributor.author | Smith, A. M. S. | |
dc.contributor.author | Southworth, J. | |
dc.contributor.author | Triaud, A. H. M. J. | |
dc.contributor.author | Udry, S. | |
dc.contributor.author | West, R. G. | |
dc.date.accessioned | 2014-09-08T13:31:02Z | |
dc.date.available | 2014-09-08T13:31:02Z | |
dc.date.issued | 2014-05-21 | |
dc.identifier.citation | Hellier , 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/stu410 | en |
dc.identifier.issn | 0035-8711 | |
dc.identifier.other | PURE: 146751493 | |
dc.identifier.other | PURE UUID: f850d7ff-c028-467a-aa18-fc0b51bbdb14 | |
dc.identifier.other | WOS: 000334744000007 | |
dc.identifier.other | Scopus: 84898809480 | |
dc.identifier.other | ORCID: /0000-0002-8863-7828/work/58531370 | |
dc.identifier.other | WOS: 000334744000007 | |
dc.identifier.uri | http://hdl.handle.net/10023/5374 | |
dc.description.abstract | We 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.extent | 11 | |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | en |
dc.rights | © 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society | en |
dc.subject | Planetary systems | en |
dc.subject | Light curves | en |
dc.subject | B 2 | en |
dc.subject | Planet | en |
dc.subject | Stars | en |
dc.subject | Superwasp | en |
dc.subject | Evolution | en |
dc.subject | QB Astronomy | en |
dc.subject | QC Physics | en |
dc.subject.lcc | QB | en |
dc.subject.lcc | QC | en |
dc.title | Transiting hot Jupiters from WASP-South, Euler and TRAPPIST : WASP-95b to WASP-101b | en |
dc.type | Journal article | en |
dc.contributor.sponsor | Science & Technology Facilities Council | en |
dc.contributor.sponsor | Science & Technology Facilities Council | en |
dc.description.version | Publisher PDF | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.identifier.doi | https://doi.org/10.1093/mnras/stu410 | |
dc.description.status | Peer reviewed | en |
dc.identifier.url | http://mnras.oxfordjournals.org/content/440/3/1982/suppl/DC1 | en |
dc.identifier.grantnumber | ST/J001651/1 | en |
dc.identifier.grantnumber | PP/F000065/1 | en |
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