Ade, Peter ![]() ![]() |
Preview |
PDF
- Published Version
Download (6MB) | Preview |
Abstract
A linear polarization field on the sphere can be uniquely decomposed into an E-mode and a B-mode component. These two components are analytically defined in terms of spin-2 spherical harmonics. Maps that contain filtered modes on a partial sky can also be decomposed into E-mode and B-mode components. However, the lack of full sky information prevents orthogonally separating these components using spherical harmonics. In this paper, we present a technique for decomposing an incomplete map into E and B-mode components using E and B eigenmodes of the pixel covariance in the observed map. This method is found to orthogonally define E and B in the presence of both partial sky coverage and spatial filtering. This method has been applied to the Bicep2 and the Keck Array maps and results in reducing E to B leakage from ΛCDM E-modes to a level corresponding to a tensor-to-scalar ratio of $r\lt 1\times {10}^{-4}$.
Item Type: | Article |
---|---|
Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Publisher: | IOP Publishing |
ISSN: | 15384357 |
Date of First Compliant Deposit: | 6 September 2017 |
Date of Acceptance: | 17 May 2016 |
Last Modified: | 05 May 2023 01:24 |
URI: | https://orca.cardiff.ac.uk/id/eprint/104400 |
Citation Data
Cited 10 times in Scopus. View in Scopus. Powered By Scopus® Data
Actions (repository staff only)
![]() |
Edit Item |