Abstract
We propose a new method to calculate Faraday rotation measure maps from multifrequency polarization angle data. In order to solve the so-called nπ-ambiguity problem which arises from the observational ambiguity of the polarization angle which is only determined up to additions of ±nπ, where n is an integer, we suggest using a global scheme. Instead of solving the nπ-ambiguity for each data point independently, our algorithm, which we chose to call PACERMAN (Polarization Angle CorrEcting Rotation Measure ANalysis), solves the nπ-ambiguity for a high signal-to-noise region 'democratically' and uses this information to assist computations in adjacent low signal-to-noise areas. © 2005 RAS.
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CITATION STYLE
Dolag, K., Vogt, C., & Enßlin, T. A. (2005). PACERMAN - I. A new algorithm to calculate Faraday rotation maps. Monthly Notices of the Royal Astronomical Society, 358(3), 726–731. https://doi.org/10.1111/j.1365-2966.2005.08851.x
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