Simultaneous uvbybeta photometric observations of the high amplitude d
elta Sct type star GP And are presented. Ten new times of light maxima
have been obtained. Using the classical O-C method, it is found that
the pulsation of this star can be well described by means of a quadrat
ic ephemeris with the period increasing at a rate of dP/Pdt = 13.0(+/-
2.8) 10(-8) y-1 over the last nineteen years. Intrinsic b - y, m1 and
c1 values are derived and the physical parameters of this star are de
termined.