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WASP-190b : tomographic discovery of a transiting hot Jupiter
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dc.contributor.author | Temple, L. Y. | |
dc.contributor.author | Hellier, C. | |
dc.contributor.author | Almleaky, Y. | |
dc.contributor.author | Anderson, D. R. | |
dc.contributor.author | Bouchy, F. | |
dc.contributor.author | Brown, D. J. A. | |
dc.contributor.author | Burdanov, A. | |
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 | Murray, C. | |
dc.contributor.author | Nielsen, L. D. | |
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 | Thompson, S. | |
dc.contributor.author | Triaud, A. H. M. J. | |
dc.contributor.author | Turner, O. D. | |
dc.contributor.author | Udry, S. | |
dc.contributor.author | West, R. G. | |
dc.date.accessioned | 2019-04-01T10:30:06Z | |
dc.date.available | 2019-04-01T10:30:06Z | |
dc.date.issued | 2019-04 | |
dc.identifier | 258412097 | |
dc.identifier | 44425240-1b0e-4ddb-808e-5f820a9c67be | |
dc.identifier | 85067821986 | |
dc.identifier | 000461452600001 | |
dc.identifier.citation | Temple , L Y , Hellier , C , Almleaky , Y , Anderson , D R , Bouchy , F , Brown , D J A , Burdanov , A , Cameron , A C , Delrez , L , Gillon , M , Jehin , E , Lendl , M , Maxted , P F L , Murray , C , Nielsen , L D , Pepe , F , Pollacco , D , Queloz , D , Ségransan , D , Smalley , B , Thompson , S , Triaud , A H M J , Turner , O D , Udry , S & West , R G 2019 , ' WASP-190b : tomographic discovery of a transiting hot Jupiter ' , Astronomical Journal , vol. 157 , no. 4 , 141 . https://doi.org/10.3847/1538-3881/ab095a | en |
dc.identifier.issn | 0004-6256 | |
dc.identifier.other | ArXiv: http://arxiv.org/abs/1811.05742v2 | |
dc.identifier.other | ORCID: /0000-0002-8863-7828/work/58531525 | |
dc.identifier.uri | https://hdl.handle.net/10023/17407 | |
dc.description | The research leading to these results has received funding from the European Research Council (ERC) under the FP/2007-2013 ERC grant agreement No. 336480, and under the H2020 ERC grant agreement No. 679030, and from an Actions de Recherche Concertée (ARC) grant, financed by the Wallonia-Brussels Federation. | en |
dc.description.abstract | We report the discovery of WASP-190b, an exoplanet on a 5.37 day orbit around a mildly evolved F6 IV-V star with V = 11.7, Teff = 6400 ± 100 K, M * = 1.35 ± 0.05 M ⊙, and R * = 1.6 ± 0.1 R ⊙. The planet has a radius of R P = 1.15 ± 0.09 R Jup and a mass of M P = 1.0 ± 0.1 M Jup, making it a mildly inflated hot Jupiter. It is the first hot Jupiter confirmed via Doppler tomography with an orbital period of >5 days. The orbit is also marginally misaligned with respect to the stellar rotation, with λ = 21° ± 6° measured using Doppler tomography. | |
dc.format.extent | 7 | |
dc.format.extent | 987945 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astronomical Journal | en |
dc.subject | Planets and satellites: detection | en |
dc.subject | Planets and satellites: individual (WASP-190b) | en |
dc.subject | Stars: individual (WASP-190) | 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-190b : tomographic discovery of a transiting hot Jupiter | en |
dc.type | Journal article | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.contributor.institution | University of St Andrews. St Andrews Centre for Exoplanet Science | en |
dc.identifier.doi | 10.3847/1538-3881/ab095a | |
dc.description.status | Peer reviewed | en |
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