  I found that ASASSN-V J205543.90+240033.5 shows large-amplitude (1.2-1.4 mag)
nearly sinusoidal variations with a period of 10.803(2) d and very short period
variations with a period of 0.0068 d using Public Data Release of Zwicky
Transient Facility observations. The only known object that shows a similar
combination of nearly sinusoidal reflection variations and very short period,
large-amplitude variations is the unique white dwarf pulsar AR Sco. ASASSN-V
J205543.90+240033.5 appears to be very similar to AR Sco and observations at
various wavelengths are desired.
