  Using numerical simulations, we investigate the distribution of Kondo
temperatures at the Anderson transition. In agreement with previous work, we
find that the distribution has a long tail at small Kondo temperatures.
Recently, an approximation for the tail of the distribution was derived
analytically. This approximation takes into account the multifractal
distribution of the wavefunction amplitudes (in the parabolic approximation),
and power law correlations between wave function intensities, at the Anderson
transition. It was predicted that the distribution of Kondo temperatures has a
power law tail with a universal exponent. Here, we attempt to check that this
prediction holds in a numerical simulation of Anderson's model of localisation
in three dimensions.
