  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
($V = 11.6$).
