WASP-190b: tomographic discovery of a transiting hot Jupiter

L. Y. Temple; C. Hellier; Y. Almleaky; D. R. Anderson; F. Bouchy; D. J. A. Brown; A. Burdanov; A. Collier Cameron; L. Delrez; M. Gillon; E. Jehin; M. Lendl; P. F. L. Maxted; C. Murray; L. D. Nielsen; F. Pepe; D. Pollacco; D. Queloz; D. Ségransan; B. Smalley; S. Thompson; A. H. M. J. Triaud; O. D. Turner; S. Udry; R. G. West

doi:10.3847/1538-3881/ab095a

WASP-190b: tomographic discovery of a transiting hot Jupiter

L. Y. Temple, C. Hellier, Y. Almleaky, D. R. Anderson, F. Bouchy, D. J. A. Brown, A. Burdanov, A. Collier Cameron, L. Delrez, M. Gillon, E. Jehin, M. Lendl, P. F. L. Maxted, C. Murray, L. D. Nielsen, F. Pepe, D. Pollacco, D. Queloz, D. Ségransan, B. SmalleyS. Thompson, A. H. M. J. Triaud, O. D. Turner, S. Udry, R. G. West

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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, T_eff = 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.

Original language	English
Article number	141
Number of pages	7
Journal	Astronomical Journal
Volume	157
Issue number	4
Early online date	14 Mar 2019
DOIs	https://doi.org/10.3847/1538-3881/ab095a
Publication status	Published - Apr 2019

Keywords

Planets and satellites: detection
Planets and satellites: individual (WASP-190b)
Stars: individual (WASP-190)

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Temple_2019_AJ_157_141
© 2019, The American Astronomical Society. This work has been made available online in accordance with the publisher's policies. This is the final published version of the work, which was originally published at https://doi.org/10.3847/1538-3881/ab095a
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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., ... West, R. G. (2019). WASP-190b: tomographic discovery of a transiting hot Jupiter. Astronomical Journal, 157(4), Article 141. https://doi.org/10.3847/1538-3881/ab095a

@article{444252401b0e4ddb808e5f820a9c67be,

title = "WASP-190b: tomographic discovery of a transiting hot Jupiter",

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.",

keywords = "Planets and satellites: detection, Planets and satellites: individual (WASP-190b), Stars: individual (WASP-190)",

author = "Temple, \{L. Y.\} and C. Hellier and Y. Almleaky and Anderson, \{D. R.\} and F. Bouchy and Brown, \{D. J. A.\} and A. Burdanov and Cameron, \{A. Collier\} and L. Delrez and M. Gillon and E. Jehin and M. Lendl and Maxted, \{P. F. L.\} and C. Murray and Nielsen, \{L. D.\} and F. Pepe and D. Pollacco and D. Queloz and D. S{\'e}gransan and B. Smalley and S. Thompson and Triaud, \{A. H. M. J.\} and Turner, \{O. D.\} and S. Udry and West, \{R. G.\}",

note = "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 Concert{\'e}e (ARC) grant, financed by the Wallonia-Brussels Federation.",

year = "2019",

month = apr,

doi = "10.3847/1538-3881/ab095a",

language = "English",

volume = "157",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "American Astronomical Society",

number = "4",

}

Temple, LY, Hellier, C, Almleaky, Y, Anderson, DR, Bouchy, F, Brown, DJA, Burdanov, A, Cameron, AC, Delrez, L, Gillon, M, Jehin, E, Lendl, M, Maxted, PFL, Murray, C, Nielsen, LD, Pepe, F, Pollacco, D, Queloz, D, Ségransan, D, Smalley, B, Thompson, S, Triaud, AHMJ, Turner, OD, Udry, S & West, RG 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

TY - JOUR

T1 - WASP-190b

T2 - tomographic discovery of a transiting hot Jupiter

AU - Temple, L. Y.

AU - Hellier, C.

AU - Almleaky, Y.

AU - Anderson, D. R.

AU - Bouchy, F.

AU - Brown, D. J. A.

AU - Burdanov, A.

AU - Cameron, A. Collier

AU - Delrez, L.

AU - Gillon, M.

AU - Jehin, E.

AU - Lendl, M.

AU - Maxted, P. F. L.

AU - Murray, C.

AU - Nielsen, L. D.

AU - Pepe, F.

AU - Pollacco, D.

AU - Queloz, D.

AU - Ségransan, D.

AU - Smalley, B.

AU - Thompson, S.

AU - Triaud, A. H. M. J.

AU - Turner, O. D.

AU - Udry, S.

AU - West, R. G.

N1 - 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.

PY - 2019/4

Y1 - 2019/4

N2 - 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.

AB - 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.

KW - Planets and satellites: detection

KW - Planets and satellites: individual (WASP-190b)

KW - Stars: individual (WASP-190)

UR - https://www.scopus.com/pages/publications/85067821986

U2 - 10.3847/1538-3881/ab095a

DO - 10.3847/1538-3881/ab095a

M3 - Article

SN - 0004-6256

VL - 157

JO - Astronomical Journal

JF - Astronomical Journal

IS - 4

M1 - 141

ER -

WASP-190b: tomographic discovery of a transiting hot Jupiter

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