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

V Vacca; N Oppermann; T A Ensslin; M Selig; H Junklewitz; M Greiner; J Jasche; C A Hales; M Reneicke; E Carretti; L Feretti; C Ferrari; G Giovannini; F Govoni; C Horellou; S Ideguchi; M Johnston-Hollitt; M Murgia; R Paladino; R Pizzo; A Scaife

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

V Vacca, N Oppermann, T A Ensslin, M Selig, H Junklewitz, M Greiner, J Jasche, C A Hales, M Reneicke, E Carretti, L Feretti, C Ferrari, G Giovannini, F Govoni, C Horellou, S Ideguchi, M Johnston-Hollitt, M Murgia, R Paladino, R PizzoA Scaife

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Abstract

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.

Original language	English
Journal	Advancing Astrophysics with the Square Kilometre Array (AASKA14)
Publication status	Published - 2015

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http://adsabs.harvard.edu/abs/2015aska.confE.114V

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Vacca, V., Oppermann, N., Ensslin, T. A., Selig, M., Junklewitz, H., Greiner, M., Jasche, J., Hales, C. A., Reneicke, M., Carretti, E., Feretti, L., Ferrari, C., Giovannini, G., Govoni, F., Horellou, C., Ideguchi, S., Johnston-Hollitt, M., Murgia, M., Paladino, R., ... Scaife, A. (2015). Statistical methods for the analysis of rotation measure grids in large scale structures in the SKA era. Advancing Astrophysics with the Square Kilometre Array (AASKA14). http://adsabs.harvard.edu/abs/2015aska.confE.114V

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title = "Statistical methods for the analysis of rotation measure grids in large scale structures in the SKA era",

abstract = "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.",

author = "V Vacca and N Oppermann and Ensslin, {T A} and M Selig and H Junklewitz and M Greiner and J Jasche and Hales, {C A} and M Reneicke and E Carretti and L Feretti and C Ferrari and G Giovannini and F Govoni and C Horellou and S Ideguchi and M Johnston-Hollitt and M Murgia and R Paladino and R Pizzo and A Scaife",

year = "2015",

language = "English",

journal = "Advancing Astrophysics with the Square Kilometre Array (AASKA14)",

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Vacca, V, Oppermann, N, Ensslin, TA, Selig, M, Junklewitz, H, Greiner, M, Jasche, J, Hales, CA, Reneicke, M, Carretti, E, Feretti, L, Ferrari, C, Giovannini, G, Govoni, F, Horellou, C, Ideguchi, S, Johnston-Hollitt, M, Murgia, M, Paladino, R, Pizzo, R & Scaife, A 2015, 'Statistical methods for the analysis of rotation measure grids in large scale structures in the SKA era', Advancing Astrophysics with the Square Kilometre Array (AASKA14). <http://adsabs.harvard.edu/abs/2015aska.confE.114V>

TY - JOUR

T1 - Statistical methods for the analysis of rotation measure grids in large scale structures in the SKA era

AU - Vacca, V

AU - Oppermann, N

AU - Ensslin, T A

AU - Selig, M

AU - Junklewitz, H

AU - Greiner, M

AU - Jasche, J

AU - Hales, C A

AU - Reneicke, M

AU - Carretti, E

AU - Feretti, L

AU - Ferrari, C

AU - Giovannini, G

AU - Govoni, F

AU - Horellou, C

AU - Ideguchi, S

AU - Johnston-Hollitt, M

AU - Murgia, M

AU - Paladino, R

AU - Pizzo, R

AU - Scaife, A

PY - 2015

Y1 - 2015

N2 - 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.

AB - 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.

M3 - Article

JO - Advancing Astrophysics with the Square Kilometre Array (AASKA14)

JF - Advancing Astrophysics with the Square Kilometre Array (AASKA14)

ER -

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

Abstract

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