  We report 3 new R Coronae Borealis and 63 new DY Persei candidates in the
Small Magellanic Cloud. Our analysis, based on data published by the OGLE team,
consisted in a search for the characteristic drops in brightness that define
these classes. All candidates had been previously classified as semi-regular or
Mira variables. We briefly remark upon the possible existence of a "borderline"
DY Per-like star and a "transitional" DY Per/RCB star. Follow-up observations
are needed to conclusively establish the nature of our candidates.
