  The physical origin of fast radio bursts (FRBs) is unknown. Young magnetars
born from gamma-ray bursts (GRBs) have been suggested to be a possible central
engine of FRBs. We test such a hypothesis by systematically searching for
GRB-FRB spatial associations from 110 FRBs and 1440 GRBs. We find that one FRB
event, FRB 171209, discovered by the Parkes telescope is spatially coincident
with a historical long-duration GRB 110715A at $z=0.82$. The afterglow of GRB
110715A is consistent with being powered by a millisecond magnetar. The
extragalactic dispersion measure of FRB 171209 is in excess of that contributed
by the intergalactic medium, which can be interpreted as being contributed by a
young supernova remnant associated with the GRB. Overall, the significance of
the association is $(2.28 - 2.55) \sigma$. If the association is indeed
physical, our result suggests that the magnetars associated with long GRBs can
be the progenitors of at least some FRBs.
