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WASP-120 b, WASP-122 b, AND WASP-123 b : three newly discovered planets from the WASP-South survey
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dc.contributor.author | Turner, O. D. | |
dc.contributor.author | Anderson, D. R. | |
dc.contributor.author | Cameron, Andrew Collier | |
dc.contributor.author | Delrez, L. | |
dc.contributor.author | Evans, D. F. | |
dc.contributor.author | Gillon, M. | |
dc.contributor.author | Hellier, C. | |
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 | Ségransan, D. | |
dc.contributor.author | Smalley, B. | |
dc.contributor.author | Smith, A. M. S. | |
dc.contributor.author | Triaud, A. H. M. J. | |
dc.contributor.author | Udry, S. | |
dc.contributor.author | West, R. G. | |
dc.date.accessioned | 2017-05-17T23:33:46Z | |
dc.date.available | 2017-05-17T23:33:46Z | |
dc.date.issued | 2016-06 | |
dc.identifier | 243086721 | |
dc.identifier | 3a545240-be34-4d45-b1ea-f222584a2dad | |
dc.identifier | 84973515274 | |
dc.identifier | 000387110500004 | |
dc.identifier.citation | Turner , O D , Anderson , D R , Cameron , A C , Delrez , L , Evans , D F , Gillon , M , Hellier , C , Jehin , E , Lendl , M , Maxted , P F L , Pepe , F , Pollacco , D , Queloz , D , Ségransan , D , Smalley , B , Smith , A M S , Triaud , A H M J , Udry , S & West , R G 2016 , ' WASP-120 b, WASP-122 b, AND WASP-123 b : three newly discovered planets from the WASP-South survey ' , Publications of the Astronomical Society of the Pacific , vol. 128 , no. 964 , 64401 . https://doi.org/10.1088/1538-3873/128/964/064401 | en |
dc.identifier.issn | 0004-6280 | |
dc.identifier.other | BibCode: 2016PASP..128f4401T | |
dc.identifier.other | ORCID: /0000-0002-8863-7828/work/58531390 | |
dc.identifier.uri | https://hdl.handle.net/10023/10795 | |
dc.description.abstract | We present the discovery by the WASP-South survey of three planets transiting moderately bright stars (V ≈ 11). WASP-120 b is a massive (4.85 M Jup) planet in a 3.6-day orbit that we find likely to be eccentric (e={0.059}-0.018+0.025) around an F5 star. WASP-122 b is a hot Jupiter (1.28 M Jup, 1.74 R Jup) in a 1.7-day orbit about a G4 star. Our predicted transit depth variation caused by the atmosphere of WASP-122 b suggests it is well suited to characterization. WASP-123 b is a hot Jupiter (0.90M Jup, 1.32 R Jup) in a 3.0-day orbit around an old (∼7 Gyr) G5 star. | |
dc.format.extent | 2098879 | |
dc.language.iso | eng | |
dc.relation.ispartof | Publications of the Astronomical Society of the Pacific | en |
dc.subject | Planetary systems | en |
dc.subject | Stars: individual (WASP-120, WASP-122, WASP-123) | en |
dc.subject | QB Astronomy | en |
dc.subject | QC Physics | en |
dc.subject | NDAS | en |
dc.subject.lcc | QB | en |
dc.subject.lcc | QC | en |
dc.title | WASP-120 b, WASP-122 b, AND WASP-123 b : three newly discovered planets from the WASP-South survey | en |
dc.type | Journal article | en |
dc.contributor.sponsor | Science & Technology Facilities Council | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.identifier.doi | 10.1088/1538-3873/128/964/064401 | |
dc.description.status | Peer reviewed | en |
dc.date.embargoedUntil | 2017-05-17 | |
dc.identifier.url | http://adsabs.harvard.edu/abs/2016PASP..128f4401T | en |
dc.identifier.grantnumber | ST/M001296/1 | en |
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