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BICEP2/KECK ARRAY. VII. MATRIX BASED E/B SEPARATION APPLIED TO BICEP2 AND THE KECK ARRAY.
- Source :
- Astrophysical Journal; 7/1/2016, Vol. 825 Issue 1, p1-1, 1p
- Publication Year :
- 2016
-
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 . [ABSTRACT FROM AUTHOR]
- Subjects :
- LINEAR polarization
SPHERICAL harmonics
BEAMFORMING
ASTRONOMY
COVARIANCE matrices
Subjects
Details
- Language :
- English
- ISSN :
- 0004637X
- Volume :
- 825
- Issue :
- 1
- Database :
- Complementary Index
- Journal :
- Astrophysical Journal
- Publication Type :
- Academic Journal
- Accession number :
- 116661005
- Full Text :
- https://doi.org/10.3847/0004-637X/825/1/66