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We report the discovery of two hot Jupiters orbiting the stars EPIC229426032and EPIC246067459. We used photometric data from Campaign 11 and 12 of theKepler K2 Mission and radial velocity data obtained using the HARPS, FEROS, andCORALIE 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 areorbiting their host stars in 2.18 and 3.20-day orbits, respectively. The largeradius of EPIC229426032 b leads us to conclude that this candidate correspondsto a highly inflated hot Jupiter. EPIC2460674559 b has a radius consistent withtheoretical 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($V = 11.6$).

EPIC229426032 b and EPIC246067459 b: discovery and characterization of two new transiting hot Jupiters from K2