  In astro-ph/0109199, the initial conditions (IC's) of cosmological N-body
simulations by the Virgo Consortium are analyzed and it is concluded that the
density fluctuations are rather different from the desired ones. We have
repeated the analysis of the IC's using our own code and the code provided by
the authors of astro-ph/0109199, obtaining results that disprove the
criticisms.
