  The present paper gives new elements for the light variations of the EA
variable star AY Peg, on the basis of new times of minimum performed visually
and with ccd by members of GEOS between 1985 and 2018, and the ASAS-SN set of
data available. On one hand, we can establish a new ephemeris with a possible
quadratic term, and on the other hand, the amplitude of the primary minimum
appears much deeper than the one given in GCVS. AY Peg varies between 13.1 and
15.6 magnitude at its primary eclipse.
