  Recently, brightness variations occurring on twice the accretion disk
precession period in the old nova and permanent superhump system V603 Aql have
been observed by Bruch & Cook (2018). In an attempt to detect a similar effect
in other cataclysmic variables reported to contain permanent superhumps the
novalike variable UU Aqr was observed during 11 nights in September 2018. While
no traces of superhumps were seen in the data, rendering the quest for
variations related to the disk precession period obsolete, the system exhibits
regular variations with a period of ~4 days.
