Orthogonal BipoSH measures : Scrutinizing sources of isotropy violation

TL;DR

This paper introduces orthogonal BipoSH estimators to distinguish between different sources of isotropy violation in the CMB, enhancing the interpretability of SI violation signals.

Contribution

The paper proposes a novel technique of orthogonal BipoSH estimators to identify specific causes of isotropy violation in the CMB.

Findings

Orthogonal BipoSH estimators can differentiate between models of isotropy violation.

The method improves the interpretability of BipoSH spectra in CMB analysis.

It provides a new tool for scrutinizing sources of anisotropy in cosmological data.

Abstract

The two point correlation function of the CMB temperature anisotropies is generally assumed to be statistically isotropic (SI). Deviations from this assumption could be traced to physical or observational artefacts and systematic effects. Measurement of non-vanishing power in the BipoSH spectra is a standard statistical technique to search for isotropy violations. Although this is a neat tool allowing a blind search for SI violations in the CMB sky, it is not easy to discern the cause of isotropy violation using this measure. In this article, we propose a novel technique of constructing orthogonal BipoSH estimators, which can be used to discern between models of isotropy violation.