Accurate Extragalactic Magnetic Fields from Faraday Rotation with Optimal Dispersion Measure Estimators

arXiv:2607.20985 · astro-ph.GA · Submitted 2026-07-23 · Read on arXiv

Hilay Shah, Mark Krumholz, Naomi McClure-Griffiths, Zipeng Hu

astro-ph.GA

Submitted: 2026-07-23

Comments: 22 pages, 10 figures, under review MNRAS

Code: https://github.com/mikegrudic/pytreegrav

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

Accuracy — 13× in this paper · explained in 1 episode
Milky Way — 9× in this paper
Calibration — 3× in this paper · explained in 7 episodes
Abundance — 2× in this paper · explained in 1 episode
Consistency — 2× in this paper · explained in 3 episodes
Fast Radio Burst — 2× in this paper
Robustness — 2× in this paper · explained in 5 episodes
Trace — 2× in this paper · explained in 2 episodes
alpha — 2× in this paper · explained in 1 episode
Adaptive Algorithm — 1× in this paper · explained in 1 episode
Degeneracy — 1× in this paper · explained in 3 episodes
Fast Radio Bursts (FRBs) — 1× in this paper · explained in 4 episodes
Large Magellanic Cloud — 1× in this paper
Magnetohydrodynamics (MHD) — 1× in this paper · explained in 3 episodes
Population Synthesis — 1× in this paper · explained in 2 episodes
Velocity Dispersion — 1× in this paper · explained in 2 episodes

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