Characterizing the Uncertainty in Cluster Magnetic Fields derived from Rotation Measures
Andrew Johnson, Lawrence Rudnick, Thomas Jones, Peter Mendygral, Klaus, Dolag

TL;DR
This paper analyzes the uncertainties in estimating galaxy cluster magnetic fields from Faraday rotation measures, revealing an irreducible factor of about 3 and key sources of uncertainty.
Contribution
It provides a formalism to quantify uncertainties in RM-based magnetic field estimates using synthetic data from cosmological simulations.
Findings
Uncertainty factor of approximately 3 in magnetic field estimates
Principal uncertainties include line-of-sight depth and coherence length
RM estimates span over an order of magnitude in synthetic experiments
Abstract
Magnetic fields play vital roles in intracluster media (ICMs), but estimating their strengths and distributions from observations is a major challenge. Faraday rotation measures (RMs) are widely applied to this task, so it is critical to understand inherent uncertainties in RM analysis. In this paper, we seek to characterize those uncertainties given the types of information available today, independent of the specific technique used. We conduct synthetic RM observations through the ICM of a galaxy cluster drawn from an MHD cosmological simulation in which the magnetic field is known. We analyze the synthetic RM observations using an analytical formalism based on commonly used model assumptions allowing us to relate model physical variables to outcome uncertainties. Despite the simplicity of some assumptions, and unknown physical parameters, we are able to extract an approximate…
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