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

Lookup NU author(s): Dr Christopher Hales

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This work is licensed under a Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0).

Abstract

© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence. 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.

Publication metadata

Author(s): Vacca V, Oppermann N, Ensslin T, Selig M, Junklewitz H, Greiner M, Jasche J, Hales CA, Reinecke M, Carretti E, Feretti L, Ferrari C, Giovannini G, Govoni F, Horellou C, Ideguchi S, Johnston-Hollitt M, Murgia M, Paladino R, Pizzo RF, Scaife A

Publication type: Conference Proceedings (inc. Abstract)

Publication status: Published

Conference Name: Advancing Astrophysics with the Square Kilometre Array

Year of Conference: 2014

Pages: 1-9

Online publication date: 09/06/2014

Acceptance date: 01/01/1900

Date deposited: 30/06/2017

Publisher: Proceedings of Science (PoS)

URL: https://pos.sissa.it/archive/conferences/215/114/AASKA14_114.pdf

Notes: Paper presented at the conference Advancing Astrophysics with the Square Kilometre Array, June 8-13, 2014, Giardini Naxos, Italy

Series Title: Proceedings of Science

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