  From sector 1--44 {\em TESS} observations, 19 new roAp stars, 103 ostensibly
non-peculiar stars with roAp-like frequencies and 617 $\delta$~Scuti stars with
independent frequencies typical of roAp stars were found. Examination of all
chemically peculiar stars observed by {\em TESS} resulted in the discovery of
199 Ap stars which pulsate as $\delta$~Sct or $\gamma$~Dor variables. The
fraction of pulsating Ap stars is the same as the fraction of pulsating
chemically normal stars. There is no distinct separation in frequency or radial
order between chemically peculiar $\delta$~Sct stars and roAp stars. In fact,
all the features which originally distinguished roAp from $\delta$~Sct stars in
the past have disappeared. There is no reason to assume that the high
frequencies in roAp stars are driven by a different mechanism from the high
frequencies in chemically normal stars. However, chemically peculiar stars are
far more likely to pulsate with high frequencies. The term "roAp" should be
dropped: all roAp stars are normal $\delta$~Scuti stars.
