Using rotation measure grids to detect cosmological magnetic fields: A Bayesian approach-Reference-Cited by-同舟云学术

Using rotation measure grids to detect cosmological magnetic fields: A Bayesian approach

Published:2016-06-03 Issue: Volume:591 Page:A13
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Vacca V.,Oppermann N.,Enßlin T.,Jasche J.,Selig M.,Greiner M.,Junklewitz H.,Reinecke M.,Brüggen M.,Carretti E.,Feretti L.,Ferrari C.,Hales C. A.,Horellou C.,Ideguchi S.,Johnston-Hollitt M.,Pizzo R. F.,Röttgering H.,Shimwell T. W.,Takahashi K.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201527291/pdf

Reference111 articles.

1. THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY

2. FARADAY ROTATION MEASURE DUE TO THE INTERGALACTIC MAGNETIC FIELD. II. THE COSMOLOGICAL CONTRIBUTION

3. STATISTICAL TECHNIQUES FOR DETECTING THE INTERGALACTIC MAGNETIC FIELD FROM LARGE SAMPLES OF EXTRAGALACTIC FARADAY ROTATION DATA

4. Exploring the intergalactic magnetic field by means of Faraday tomography

5. Evidence for shock acceleration and intergalactic magnetic fields in a large-scale filament of galaxies ZwCl 2341.1+0000

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