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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4924

Title: Galactic dust polarized emission at high latitudes and CMB polarization
Authors: Sethi, S.K.
Prunet, S.
Bouchet, F.R.
Issue Date: Mar-1998
Publisher: EDP Sciences
Citation: Astronomy and Astrophysics, 1998, Vol.339, p187
Abstract: We estimate the dust polarized emission in our galaxy at high galactic latitudes, which is the dominant foreground for measuring CMB polarization using the high frequency instrument (HFI) aboard Planck surveyor. We compare it with the level of CMB polarization and conclude that, for angular scales $\le 1^{\circ}$, the scalar-induced CMB polarization and temperature-polarization cross-correlation are much larger than the foreground level at $\nu \simeq 100 GHz$. The tensor-induced signals seem to be at best comparable to the foreground level.}
Description: Open Access
URI: http://hdl.handle.net/2289/4924
ISSN: 0004-6361
1432-0746 (Online)
Alternative Location: http://adsabs.harvard.edu/abs/1998astro.ph..3158S
http://arxiv.org/abs/astro-ph/9803158
http://dx.doi.org/
Copyright: 1998 EDP Sciences
Appears in Collections:Research Papers (A&A)

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