  The light curve of the cataclismic variable ASASSN-18aan is studied using
recent observations of the MC589 Observatory, giving an orbital Period and
Epoch fully consistent with the data obtained after the discovery flare in
2018. Archival data from ASASSN, ZTF and Gaia were used to check if its flares
have a quasi-periodic behaviour. A recurrency time scale of about 11 months is
found, confirming a previous tentative result using the historic plate archive
of the Asiago Observatory. The next outbursts are expected by April 2023 and
March 2024.
