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Galactic Foregrounds and CMB Polarization with SPOrt

Published online by Cambridge University Press:  26 May 2016

M. Tucci ,
S. Cortiglioni ,
E. Carretti ,
M. Orsini ,
R. Fabbri ,
S. Cecchini ,
G. Sironi ,
G. Boella ,
S. Bonometto  and
M. Gervasi
...Show all authors
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

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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
Information
Symposium - International Astronomical Union , Volume 201: New Cosmological Data and the Values of the Fundamental Parameters , 2005 , pp. 523 - 524
Copyright
Copyright © Astronomical Society of the Pacific 2005 

References

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