The low large-scale CMB variance, concentrated away from the Galactic plane, remains anomalous at about 2.8 to 3 sigma even after random rotations of the sky are taken into account.
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Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane?
The low large-scale CMB variance, concentrated away from the Galactic plane, remains anomalous at about 2.8 to 3 sigma even after random rotations of the sky are taken into account.