Eight Exoplanet Candidates in SAO Survey

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