  We performed a careful numerical analysis of the late tail behaviour of waves
propagating in the Schwarzschild spacetime. Specifically the scalar monopole,
the electromagnetic dipole and the gravitational axial quadrupole waves have
been investigated. The obtained results agree with a falloff $1/t^{2l+3}$ for
the general initial data and $1/t^{2l+4}$ for the initially static data.
