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BICEP2/KECK ARRAY. VII. MATRIX BASED E/B SEPARATION APPLIED TO BICEP2 AND THE KECK ARRAY.

Authors :
P. A. R. Ade
Z. Ahmed
R. W. Aikin
K. D. Alexander
D. Barkats
S. J. Benton
C. A. Bischoff
J. J. Bock
R. Bowens-Rubin
J. A. Brevik
I. Buder
E. Bullock
V. Buza
J. Connors
B. P. Crill
L. Duband
C. Dvorkin
J. P. Filippini
S. Fliescher
J. Grayson
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]

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