Table 6
Summary of results in this paper.
| Anomaly | After sparse | After ISW |
| inpainting | subtraction | |
|
|
||
| Low quad | More anomalous | More anomalous |
| Quad/oct | Less anomalous | Less anomalous |
| alignment | ||
| Oct planarity | Less anomalous | Less anomalous |
Notes. We identify trends from the 11 WMAP data sets described in Table 1 regarding how sparse inpainting and subtraction of the ISW signal due to 2MASS and NVSS galaxies can affect the three anomalies investigated. The third test for octopole planarity did not return significantly anomalous results in the first place.
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