A new polarization amplitude bias reduction method
Author
dc.contributor.author
Vidal, Matías
Author
dc.contributor.author
Leahy, J. P.
Author
dc.contributor.author
Dickinson, C.
Admission date
dc.date.accessioned
2017-03-02T14:13:15Z
Available date
dc.date.available
2017-03-02T14:13:15Z
Publication date
dc.date.issued
2016
Cita de ítem
dc.identifier.citation
Monthly Notices of The Royal Astronomical Society. Volumen: 461 Número: 1 Páginas: 698-709
es_ES
Identifier
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10.1093/mnras/stw1298
Identifier
dc.identifier.uri
https://repositorio.uchile.cl/handle/2250/142940
Abstract
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Polarization amplitude estimation is affected by a positive noise bias, particularly important in regions with low signal-to-noise ratio (SNR). We present a new approach to correct for this bias in the case there is additional information about the polarization angle. We develop the 'known-angle estimator' that works in the special case when there is an independent and high SNR (greater than or similar to 2 sigma) measurement of the polarization angle. It is derived for the general case where the uncertainties in the Q, U Stokes parameters are not symmetric. This estimator completely corrects for the polarization bias if the polarization angle is perfectly known. In the realistic case, where the angle template has uncertainties, a small residual bias remains, but that is shown to be much smaller that the one left by other classical estimators. We also test our method with more realistic data, using the noise properties of the three lower frequency maps of Wilkinson Microwave Anisotropy Probe. In this case, the known-angle estimator also produces better results than methods that do not include the angle information. This estimator is therefore useful in the case where the polarization angle is expected to be constant over different data sets with different SNR.