We report the discovery of two hot Jupiters orbiting the stars EPIC229426032 and EPIC246067459 .
We used photometric data from Campaign 11 and 12 of the Kepler K2 Mission and radial velocity data obtained using the HARPS , FEROS , and CORALIE spectrographs .
EPIC229426032 b and EPIC246067459 b have masses of 1.60 ^ { +0.11 } _ { -0.11 } and 0.86 ^ { +0.13 } _ { -0.12 } M _ { \mathrm { Jup } } , radii of 1.65 ^ { +0.07 } _ { -0.08 } and 1.30 ^ { +0.15 } _ { -0.14 } R _ { \mathrm { Jup } } , and are orbiting their host stars in 2.18 and 3.20-day orbits , respectively .
The large radius of EPIC229426032 b leads us to conclude that this candidate corresponds to a highly inflated hot Jupiter .
EPIC2460674559 b has a radius consistent with theoretical models , considering the high incident flux falling on the planet .
We consider EPIC229426032 b to be a excellent system for follow-up studies , since not only is it very inflated , but it also orbits a relatively bright star ( V = 11.6 ) .