Advances in Astronomy / 2010 / Article / Fig 6

Review Article

Large-Angle Anomalies in the CMB

Figure 6

The two-point angular correlation function from the WMAP 5-year results. Plotted are for the ILC calculated separately on the part of the sky outside the KQ75 cut (dashed line), inside the KQ75 cut (dotted line), and on the part of the sky with at least on point inside the KQ75 cut (dotted-dashed line). For better comparison to the full-sky (solid line), the partial sky has been scaled by the fraction of the sky over which they are calculated. Adopted from [31].