  Spectroscopic observations are extremely important for determining the
composition, structure, and surface gravity of exoplanetary atmospheres. High
resolution spectroscopy of the planet itself has only been demonstrated a
handful of times. By using advanced high contrast imagers, it is possible to
conduct high resolution spectroscopy on imageable exoplanets, after the star
light is first suppressed with an advanced coronagraph. Because the planet is
spatially separated in the focal plane, a single mode fiber could be used to
collect the light from the planet alone, reducing the photon noise by orders of
magnitude. In addition, speckle control applied to the location where an
exoplanet is known to exist, can be used to preferentially reject the stellar
flux from the fiber further.
  In this paper we will present the plans for conducting high resolution
spectroscopic studies of this nature with the combination of SCExAO and IRD in
the H-band on the Subaru Telescope. This technique will be critical to the
characterization of terrestrial planets on ELTs and future space missions.
