Application of the Kolmogorov-Smirnov test to CMB data: Is the universe
  really weakly random?
  A recent application of the Kolmogorov-Smirnov test to the WMAP 7 year W-band
maps claims evidence that the CMB is "weakly random", and that only 20% of the
signal can be explained as a random Gaussian field. I here repeat this
analysis, and in contrast to the original result find no evidence for deviation
from the standard {\Lambda}CDM model. Instead, the results of the original
analysis are consistent with not properly taking into account the correlations
of the {\Lambda}CDM power spectrum.
