
TL;DR
This paper investigates the North-South asymmetry in large-angle CMB correlations, demonstrating it is unrelated to quadrupole-octopole alignment and analyzing its dependence on data processing and sky masks.
Contribution
It provides evidence that the North-South asymmetry is independent of low multipole alignments and examines how data masks influence its statistical significance.
Findings
North-South asymmetry exists in multipoles 4-10.
Asymmetry significance varies with data set and masks.
Asymmetry is unrelated to quadrupole-octopole alignment.
Abstract
Several accurate analyses have revealed a statistically significant North-South ecliptic asymmetry in the large-angle correlations strength of the Cosmic Microwave Background (CMB) radiation temperature field data from the Wilkinson Microwave Anisotropy Probe (WMAP). This asymmetry is inconsistent with the statistical isotropy expected in the concordance cosmological model LCDM. It has been suggested that a possible cause-effect relationship exists between this large-angle anisotropy and the anomalous CMB quadrupole-octopole planes alignment. In turn, this later phenomenon (or both) would be a consequence of one or more of the following undesired effects in CMB data: a systematic error in the data processing or in the instrument characterization, residual foregrounds, and large-angle correlations induced by the incomplete sky CMB data (cut-sky masks are needed to reject Galactic…
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