  We report the discovery and confirmation of two sub-Saturn planets orbiting a
bright (V = 11.3), metal-rich ([Fe/H] = 0.42 $\pm$ 0.04 dex) G3 dwarf in the K2
Campaign 2 field. The planets are 5.68 $\pm$ 0.56 Earth-radii and 7.82 $\pm$
0.72 Earth-radii and have orbital periods of 20.8851 $\pm$ 0.0003 d and
42.3633$\pm$0.0006 d, near to the 2:1 mean-motion resonance. We obtained 32
radial velocities (RVs) with Keck/HIRES and detected the reflex motion due to
EPIC-203771098b and c. These planets have masses of 21.0 $\pm$ 5.4 Earth-masses
and 27.0 $\pm$ 6.9 Earth-masses, respectively. With low densities of 0.63 $\pm$
0.25 g/cc and 0.31 $\pm$ 0.12 g/cc, respectively, the planets require thick
envelopes of H/He to explain their large sizes and low masses. Interior
structure models predict that the planets have fairly massive cores of 17.6
$\pm$ 4.3 Earth-masses and 16.1 $\pm$ 4.2 Earth-masses, respectively. They may
have formed exterior to their present locations, accreted their H/He envelopes
at large orbital distances, and migrated in as a resonant pair. The proximity
to resonance, large transit depths, and host star brightness offer rich
opportunities for TTV follow-up. Finally, the low surface gravities of the
EPIC-203771098 planets make them favorable targets for transmission
spectroscopy by HST, Spitzer, and JWST.
