Pacman (I): A new Algorithm to calculate Faraday Rotation Maps
Astrophysics
2009-11-10 v2
Abstract
We propose a new method to calculate Faraday rotation measure maps from multi-frequency polarisation angle data. In order to solve the so called n-pi ambiguity problem which arises from the observationally ambiguity of the polarisation angle which is only determined up to additions of +-n*pi, where n is an integer, we suggest using a global scheme. Instead of solving the n-pi ambiguity for each data point independently, our algorithm, which we chose to call "Pacman" (Polarisation Angle Correcting rotation Measure ANalysis), solves the n-pi ambiguity for a high signal-to-noise region ``democratically'' and uses this information to assist computations in adjacent low signal-to-noise areas.
Cite
@article{arxiv.astro-ph/0401214,
title = {Pacman (I): A new Algorithm to calculate Faraday Rotation Maps},
author = {K. Dolag and C. Vogt and T. A. Ensslin},
journal= {arXiv preprint arXiv:astro-ph/0401214},
year = {2009}
}
Comments
revised version, accepted, MNRAS in press