Angular power spectrum of the fastica cosmic microwave background component from Background Emission Anisotropy Scanning Telescope data-Reference-Cited by-同舟云学术

Angular power spectrum of the fastica cosmic microwave background component from Background Emission Anisotropy Scanning Telescope data

Published:2006-05-08 Issue:1 Volume:369 Page:441-448
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Donzelli S.,Maino D.,Bersanelli M.,Childers J.,Figueiredo N.,Lubin P. M.,Meinhold P. R.,O'Dwyer I. J.,Seiffert M. D.,Villela T.,Wandelt B. D.,Wuensche C. A.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/369/1/441/18674366/mnras0369-0441.pdf

Reference23 articles.

1. Neural networks and the separation of cosmic microwave background and astrophysical signals in sky maps

2. First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Foreground Emission

3. Multifrequency Wiener filtering of cosmic microwave background data with polarization

4. The Background Emission Anisotropy Scanning Telescope (BEAST) Instrument Description and Performances

5. Independent component analysis, A new concept?

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