  We search for transits around all known pulsating {\delta} Sct variables
(6500 K < Teff < 10 000 K) in the long-cadence Kepler data after subtracting
the pulsation signal through an automated routine. To achieve this, we devise a
simple and computationally inexpensive method for distinguishing between
low-frequency pulsations and transits in light curves. We find 3 new candidate
transit events that were previously hidden behind the pulsations, but caution
that they are likely to be false positive events. We also examined the Kepler
Objects of Interest catalog and identify 13 additional host stars which show
{\delta} Sct pulsations. For each star in our sample, we use the non-detection
of pulsation timing variations for a planet that is known to be transiting a
{\delta} Sct variable to obtain both an upper limit on the mass of the planet
and the expected radial velocity semi-amplitude of the host star. Simple
injection tests of our pipeline imply 100% recovery for planets of 0.5 RJup or
greater. Extrapolating our number of Kepler {\delta} Sct stars, we expect 12
detectable planets above 0.5 RJup in TESS. Our sample contains some of the
hottest known transiting planets around evolved stars, and is the first
complete sample of transits around {\delta} Sct variables. We make available
our code and pulsation-subtracted light curves to facilitate further analysis.
