  The purpose of this work is to supplement the "Stars with solar-type
activity" catalog with information about confirmed exoplanets and exoplanet
candidates. To do this, cross-identification of the catalog stars with data
from the NASA exoplanet archive was carried out. This article presents the
distribution of the number of suspected stars with exoplanets by brightness,
spectral type, amplitude of variability, as well as other statistical analysis
data. Particular attention has been paid to the comparison of the periods of
rotation of stars and the orbital periods of revolution of exoplanets around
them. Analysis of the data suggests the need to change the previously
determined types of variability in some stars.
