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A&A 401, 1215-1222 (2003)
DOI: 10.1051/0004-6361:20030200
An iterative destriping technique for diffuse background polarization data
C. Sbarra1, E. Carretti1, S. Cortiglioni1, M. Zannoni2, R. Fabbri3, C. Macculi1 and M. Tucci41 IASF-CNR Bologna, via P. Gobetti 101, 40129 Bologna, Italy
e-mail: carretti@bo.iasf.cnr.it; cortiglioni@bo.iasf.cnr.it; macculi@bo.iasf.cnr.it
2 IASF-CNR Milano, via Bassini 15, 20133 Milano, Italy
e-mail: zannoni@mi.iasf.cnr.it
3 Dipartimento di Fisica, Università di Firenze, via Sansone 1, 50019 Sesto Fiorentino, Italy
e-mail: fabbrir@unifi.it
4 Instituto de Fisica de Cantabria, Avda. Los Castros s/n, 39005 Santander, Spain
e-mail: tucci@ifca.unican.es
(Received 18 December 2002 / Accepted 13 February 2003)
Abstract
We describe a simple but effective iterative procedure
specifically designed to destripe
Q and
U Stokes parameter data as those collected
by the SPOrt experiment onboard the International Space Station (ISS).
The method is general enough to be useful for other experiments, both
in polarization and total intensity.
The only requirement for the algorithm to work properly is that the
receiver knee frequency must be lower than the
signal modulation frequency, corresponding in our case
to the ISS orbit period.
Detailed performances of the technique are presented in the
context of the SPOrt experiment, both in terms of added rms noise
and residual correlated noise.
Key words: cosmic microwave background -- polarization -- cosmology: observations -- methods: data analysis -- methods: numerical
Offprint request: C. Sbarra, sbarra@bo.iasf.cnr.it
© ESO 2003
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