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K2-260 b: a hot Jupiter transiting an F star, and K2-261 b: a warm Saturn around a bright G star

MPS-Authors

Johnson,  M. C.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Dai,  F.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Justesen,  A. B.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Gandolfi,  D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Hatzes,  A. P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Nowak,  G.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Endl,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Cochran,  W. D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Hidalgo,  D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Watanabe,  N.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Parviainen,  H.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Hirano,  T.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Villanueva,  S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Prieto-Arranz,  J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Narita,  N.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Palle,  E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Guenther,  E. W.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Barragán,  O.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Trifonov,  T.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Niraula,  P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

MacQueen,  P. J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Cabrera,  J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Csizmadia,  Sz
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Eigmüller,  Ph
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Grziwa,  S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Korth,  J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Pätzold,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Smith,  A. M. S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Albrecht,  S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Alonso,  R.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Deeg,  H.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Erikson,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Esposito,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Fridlund,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Fukui,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Kusakabe,  N.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Kuzuhara,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Livingston,  J.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Montañes Rodriguez,  P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Nespral,  D.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Persson,  C. M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Purismo,  T.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Raimundo,  S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Rauer,  H.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ribas,  I.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Tamura,  M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Van Eylen,  V.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Winn,  J. N.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

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Citation

Johnson, M. C., Dai, F., Justesen, A. B., Gandolfi, D., Hatzes, A. P., Nowak, G., et al. (2018). K2-260 b: a hot Jupiter transiting an F star, and K2-261 b: a warm Saturn around a bright G star. Monthly Notices of the Royal Astronomical Society, 481, 596-612.


Cite as: https://hdl.handle.net/21.11116/0000-0005-CD02-2
Abstract
We present the discovery and confirmation of two new transiting giant planets from the Kepler extended mission K2. K2-260 b is a hot Jupiter transiting a V = 12.7 F6V star in K2 Field 13, with a mass and radius of M = 1.39_{-0.06}^{+0.05} M_{☉} and R = 1.69 ± 0.03 R_{☉}. The planet has an orbital period of P = 2.627 d, and a mass and radius of M_P=1.42^{+0.31}_{-0.32} M_J and R_P=1.552^{+0.048}_{-0.057} R_J. This is the first K2 hot Jupiter with a detected secondary eclipse in the Kepler bandpass, with a depth of 71 ± 15 ppm, which we use to estimate a geometric albedo of Ag ̃ 0.2. We also detected a candidate stellar companion at 0.6 arcsec from K2-260; we find that it is very likely physically associated with the system, in which case it would be an M5-6V star at a projected separation of ̃400 au. K2-261 b is a warm Saturn transiting a bright (V = 10.5) G7IV/V star in K2 Field 14. The host star is a metal rich ([Fe/H] = 0.36 ± 0.06), mildly evolved 1.10_{-0.02}^{+0.01} M_{☉} star with R = 1.65 ± 0.04 R_{☉}. Thanks to its location near the main-sequence turn-off, we can measure a relatively precise age of 8.8_{-0.3}^{+0.4} Gyr. The planet has P = 11.633 d, MP = 0.223 ± 0.031 M_J, and R_P=0.850^{+0.026}_{-0.022} R_J, and its orbit is eccentric (e=0.39 ± 0.15). Its brightness and relatively large transit depth make this one of the best-known warm Saturns for follow-up observations to further characterize the planetary system.