  Two recent papers have claimed detection of non-Gaussian features in the COBE
DMR sky maps of the cosmic microwave background. We confirm these results, but
argue that Gaussianity is still not convincingly ruled out. Since a score of
non-Gaussianity tests have now been published, one might expect some mildly
significant results even by chance. Moreover, in the case of one measure which
yields a detection, a bispectrum statistic, we find that if the non-Gaussian
feature is real, it may well be due to detector noise rather than a
non-Gaussian sky signal, since a signal-to-noise analysis localizes it to
angular scales smaller than the beam. We study its spatial origin in case it is
nonetheless due to a sky signal (eg, a cosmic string wake or flat-spectrum
foreground contaminant). It appears highly localized in the direction b=39.5,
l=257, since removing a mere 5 pixels inside a single COBE beam area centered
there makes the effect statistically insignificant. We also test Guassianity
with an eigenmode analysis which allows a sky map to be treated as a random
number generator. A battery of tests of this generator all yield results
consistent with Gaussianity.
