Destriping of polarized data in a CMB mission with a circular
scanning
strategy
B. Revenu1, A. Kim1, R. Ansari2, F. Couchot2, J. Delabrouille1,
and J. Kaplan1
1 Physique Corpusculaire et Cosmologie, Collège de France,
11 place Marcelin Berthelot, 75231 Paris Cedex 05, France
2 Laboratoire de l'Accélérateur Linéaire, IN2P3 CNRS, Université Paris Sud,
91405 Orsay, France
Astron. Astrophys. Suppl. Ser. 142 (2000) 499-509
New caption of Fig. 8: The Mollweide projection of the residuals of the I-Stokes
parameter after destriping of 1/f noise plus white noise with
New caption of Fig. 9: The Mollweide projection of the residuals of the I-Stokes
parameter after zeroing the average of the circles, for 1/f noise plus white noise with
New caption of Fig. 10: The Mollweide projection of the residuals of the Q-Stokes parameter for a white noise mission


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