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BICEP2 / Keck Array VII: Matrix based E/B Separation applied to BICEP2 and the Keck Array

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arxiv 1603.05976 v2 pith:ZEFUU5GB submitted 2016-03-18 astro-ph.IM astro-ph.CO

Keck Array , BICEP2 Collaborations: P. Ade , Z. Ahmed , R. W. Aikin , K. D. Alexander , D. Barkats , S. J. Benton , C. A. Bischoff
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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 M. Halpern S. Harrison S. R. Hildebrandt G. C. Hilton H. Hui K. D. Irwin J. Kang K. S. Karkare E. Karpel J. P. Kaufman B. G. Keating S. Kefeli S. A. Kernasovskiy J. Kovac C. L. Kuo E. M. Leitch M. Lueker K. G. Megerian T. Namikawa C. B. Netterfield H. T. Nguyen R. O'Brient R. W. IV A. Orlando C. Pryke S. Richter R. Schwarz C. D. Sheehy Z. K. Staniszewski B. Steinbach R. V. Sudiwala G. P. Teply K. L. Thompson J. E. Tolan C. Tucker A. D. Turner A. G. Vieregg A. C. Weber D. V. Wiebe J. Willmert C. L. Wong W. L. K. Wu K. W. Yoon
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keywords componentsarrayb-modebicep2keckapplieddecomposede-mode
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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 LCDM E-modes to a level corresponding to a tensor-to-scalar ratio of $r<1\times10^{-4}$.

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Cited by 2 Pith papers

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    A new 296-detector 90 GHz TES bolometer array for CLASS achieves uniform properties, 16 μK√s NET, 0.37 optical efficiency, and a 41% mapping speed boost after addressing blue-leak radiation.

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