\_spec\], filter kernels derived with both algorithms for point sources (i.e. with beam profiles of the respective [[*Planck*]{}]{}-channels) are compared, that have been optimised for the detection of varying spectral behaviour of the signal, in this case the thermal SZ-effect, the kinetic SZ-effect and a Planckian thermal emitter with a surface temperature $T_\mathrm{surface}$ of 000 K, such as an asteroid or planet. The filter kernels depicted correspond to observing frequencies of $\nu=000$ GHz and $\nu=000$ GHz. 