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arxiv: 1501.00415 · v1 · submitted 2015-01-02 · 🌌 astro-ph.CO

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Statistical methods for the analysis of rotation measure grids in large scale structures in the SKA era

Valentina Vacca , Niels Oppermann , Torsten Ensslin , Marco Selig , Henrik Junklewitz , Maksim Greiner , Jens Jasche , Christopher Hales
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Martin Reinecke Ettore Carretti Luigina Feretti Chiara Ferrari Gabriele Giovannini Federica Govoni Cathy Horellou Shinsuke Ideguchi Melanie Johnston-Hollitt Matteo Murgia Rosita Paladino Roberto Francesco Pizzo Scaife Anna
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classification 🌌 astro-ph.CO
keywords fieldsmagneticlargemeasurerotationstatisticalanalysisapproach
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To better understand the origin and properties of cosmological magnetic fields, a detailed knowledge of magnetic fields in the large-scale structure of the Universe (galaxy clusters, filaments) is crucial. We propose a new statistical approach to study magnetic fields on large scales with the rotation measure grid data that will be obtained with the new generation of radio interferometers.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. DEFROST: Detecting Excess in Faraday Rotation thrOugh Sophisticated analysis Techniques

    astro-ph.IM 2026-05 conditional novelty 7.0

    DEFROST algorithm disentangles Galactic and extragalactic Faraday rotation in RM catalogs, recovering extragalactic parameters within 5 sigma for sources at absolute Galactic latitude above 45 degrees.