  In light of the three-year data release from WMAP we re-examine the evidence
for the ``Axis of Evil'' (AOE). We discover that previous statistics are not
robust with respect to the data-sets available and different treatments of the
galactic plane. We identify the cause of the instability and implement an
alternative ``model selection'' approach. A comparison to Gaussian isotropic
simulations find the features significant at the 94-98% level, depending on the
particular AOE model. The Bayesian evidence finds lower significance, ranging
from ``substantial'' at $\Delta(\ln E)\sim 1.4$, to no evidence for the most
general AOE model.
