PACERMAN- I. A new algorithm to calculate Faraday rotation maps
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.
- Publication:
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Monthly Notices of the Royal Astronomical Society
- Pub Date:
- April 2005
- DOI:
- arXiv:
- arXiv:astro-ph/0401214
- Bibcode:
- 2005MNRAS.358..726D
- Keywords:
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- galaxies: clusters: general;
- intergalactic medium;
- Astrophysics
- E-Print:
- revised version, accepted, MNRAS in press