  We verify candidate hypervelocity red clump stars located in the Galactic
bulge that were selected based on the VVV and the Gaia DR2 data by Luna et al.
(2019). To do so, we analyze data from the OGLE-IV survey: difference images
and astrometric time series. We have data for 30 stars out of 34 hypervelocity
candidates. We confirmed high proper motion of only one of these stars and find
out that it is a nearby one, hence, not hypervelocity. To sum up, we do not
confirm the candidate stars as hypervelocity ones. Hence, we disprove the
production rate of hypervelocity red clump stars by the central supermassive
black hole provided by Luna et al. (2019).
