  Before the launch of the Kepler Space Telescope, most studies of the rapidly
oscillating Ap (roAp) stars were conducted with ground-based photometric $B$
observations, supplemented with high-resolution time-resolved spectroscopy and
some space observations with the WIRE, MOST and BRITE satellites. These modes
of observation often only provided information on a single star at a time,
however, Kepler provided the opportunity to observe hundreds of thousands of
stars simultaneously. Over the duration of the primary 4-yr Kepler mission, and
its 4-yr reconfigured K2 mission, the telescope observed at least 14 new and
known roAp stars. This paper provides a summary the results of these
observations, including a first look at the entire data sets, and provides a
look forward to NASA's TESS mission.
