K2-237 b and K2-238 b: Discovery and characterization of two new transiting hot Jupiters from K2
Author
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Soto, M.
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Díaz, M.
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Jenkins, James Stewart
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Rojas, F.
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Espinoza, N.
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Brahm, R.
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Drass, H.
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Jones, M.
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Rabus, M.
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Hartman, J.
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Sarkis, P.
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Jordán, A.
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Lachaume, R.
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Pantoja, B.
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Vučković, M.
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Ciardi, D.
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Crossfield, I.
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Dressing, C.
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Gonzales, E.
Author
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Hirsch, L.
Admission date
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2019-05-31T15:19:56Z
Available date
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2019-05-31T15:19:56Z
Publication date
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2018
Cita de ítem
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Monthly Notices of the Royal Astronomical Society, Volumen 478, Issue 4, 2018, Pages 5356-5365
Identifier
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13652966
Identifier
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00358711
Identifier
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10.1093/mnras/sty1334
Identifier
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https://repositorio.uchile.cl/handle/2250/169400
Abstract
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We report the discovery of two hot Jupiters orbiting the stars K2-237 and K2-238. We used photometric data from Campaigns 11 and 12 of the Kepler K2 mission and radial velocity data obtained using the HARPS, FEROS, and CORALIE spectrographs. K2-237 b and K2-238 b have masses of 1.60-0.11 +0.11 and 0.86+-0.12 0.13MJup, radii of 1.65-0.08 +0.07 and 1.30-0.14 +0.15 RJup, and are orbiting their host stars in 2.18-and 3.20-d orbits, respectively. The large radius of K2-237 b leads us to conclude that this candidate corresponds to a highly inflated hot Jupiter. K2-238 b has a radius consistent with theoretical models, considering the high incident flux falling on the planet. We consider K2-237 b to be an excellent system for follow-up studies, since not only is it very inflated, but it also orbits a relatively bright star (V = 11.6).