  Here we present eight new candidates for exoplanets detected by the transit
method at the Special Astrophysical Observatory of the Russian Academy of
Sciences. Photometric observations were performed with a 50-cm robotic
telescope during the second half of 2020. We detected transits with depths of
$\Delta m = 0.056-0.173^m$ and periods $P = 18.8^h-8.3^d$ in the light curves
of stars with magnitudes of $m = 14.3-18.8^m$. All considered stars are
classified as dwarfs with radii of $R_* = 0.4-0.6 R_{sun}$ (with the
uncertainty for one star up to $1.1 R_{sun}$). We estimated the candidate radii
(all are greater than 1.4 times the Jovian radius), semi-major axes of their
orbits ($0.012-0.035 AU$), and other orbital parameters by modelling. We report
the light curves with transits for two stars obtained in 2022 based on
individual observations.
