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Galactic Foregrounds and CMB Polarization with SPOrt

  • M. Tucci (a1), S. Cortiglioni (a2), E. Carretti (a2), M. Orsini (a2), R. Fabbri (a3), S. Cecchini (a2), G. Sironi (a1), G. Boella (a1), S. Bonometto (a1), M. Gervasi (a1), C. MacCuli (a2), J. Monari (a4), L. Nicastro (a5), A. Orfei (a4), U. Pisani (a6), S. Poppi (a2), R. Tascone (a6) and M. Zannoni (a1)...


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.



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Dodelson, S. 1995, ApJ, 482, 577.
Kogut, A. et al. 1996, ApJL, 464, L5.
Tucci, M. et al. 2000, New Astronomy, 5, 181.


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