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Galactic Foregrounds and CMB Polarization with SPOrt

Published online by Cambridge University Press:  26 May 2016


M. Tucci
Affiliation:
1Physics Dept, Milano-Bicocca Univ
S. Cortiglioni
Affiliation:
2TESRE, CNR Bologna, Italy
E. Carretti
Affiliation:
2TESRE, CNR Bologna, Italy
M. Orsini
Affiliation:
2TESRE, CNR Bologna, Italy
R. Fabbri
Affiliation:
3Physics Dept., Florence University
S. Cecchini
Affiliation:
2TESRE, CNR Bologna, Italy
G. Sironi
Affiliation:
1Physics Dept, Milano-Bicocca Univ
G. Boella
Affiliation:
1Physics Dept, Milano-Bicocca Univ
S. Bonometto
Affiliation:
1Physics Dept, Milano-Bicocca Univ
M. Gervasi
Affiliation:
1Physics Dept, Milano-Bicocca Univ
C. MacCuli
Affiliation:
2TESRE, CNR Bologna, Italy
J. Monari
Affiliation:
4IRA, CNR Bologna, Italy
L. Nicastro
Affiliation:
5IFCAI, CNR Palermo
A. Orfei
Affiliation:
4IRA, CNR Bologna, Italy
U. Pisani
Affiliation:
6IRITI, CNR Turin, Italy
S. Poppi
Affiliation:
2TESRE, CNR Bologna, Italy
R. Tascone
Affiliation:
6IRITI, CNR Turin, Italy
M. Zannoni
Affiliation:
1Physics Dept, Milano-Bicocca Univ


Abstract

We discuss the expected polarization of the Galactic foregrounds at the SPOrt experiment frequencies 22-90 GHz. We also consider the problem of foreground separation and perform an analysis to estimate their impact on the detection of a cosmological signal.


Type
Part XII: Poster Papers
Copyright
Copyright © Astronomical Society of the Pacific 2005 

References

Carretti, E. et al. 2000, these proceedings, 408.Google Scholar
Dodelson, S. 1995, ApJ, 482, 577.CrossRefGoogle Scholar
Kogut, A. et al. 1996, ApJL, 464, L5.CrossRefGoogle Scholar
Tucci, M. et al. 2000, New Astronomy, 5, 181.CrossRefGoogle Scholar

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