Two Hot Jupiters from K2 Campaign 4
arXiv:1601.07844 · doi:10.3847/0004-6256/151/6/171
Abstract
We confirm the planetary nature of two transiting hot Jupiters discovered by the Kepler spacecraft's K2 extended mission in its Campaign 4, using precise radial velocity measurements from FIES@NOT, HARPS-N@TNG, and the coudé spectrograph on the McDonald Observatory 2.7 m telescope. K2-29 b (EPIC 211089792 b) transits a K1V star with a period of days; its orbit is slightly eccentric (). It has a radius of and a mass of . Its host star exhibits significant rotational variability, and we measure a rotation period of days. K2-30 b (EPIC 210957318 b) transits a G6V star with a period of days. It has a radius of and a mass of . The star has a low metallicity for a hot Jupiter host, .
Accepted for publication in AJ. 11 pages, 3 figures
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