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Techinques and algorithmic advances in the SKA era

Published online by Cambridge University Press:  03 March 2020

V. Vacca ,
F. Govoni ,
M. Murgia ,
T. Enßlin ,
N. Oppermann ,
L. Feretti ,
G. Giovannini ,
J. Jasche ,
H. Junklewitz  and
F. Loi
V. Vacca
Affiliation:
INAF - Osservatorio Astronomico di Cagliari, Via della Scienza 5, Selargius, Italy email: [email protected]
F. Govoni
Affiliation:
INAF - Osservatorio Astronomico di Cagliari, Via della Scienza 5, Selargius, Italy email: [email protected]
M. Murgia
Affiliation:
INAF - Osservatorio Astronomico di Cagliari, Via della Scienza 5, Selargius, Italy email: [email protected]
T. Enßlin
Affiliation:
MPA, Karl-Schwarzschild-Str 1, Garching, Germany
N. Oppermann
Affiliation:
CITA, University of Toronto, 60 St. George Street, Toronto, Canada
L. Feretti
Affiliation:
INAF - Istituto di Radioastronomia, Via Gobetti 101, Bologna, Italy
G. Giovannini
Affiliation:
INAF - Istituto di Radioastronomia, Via Gobetti 101, Bologna, Italy DIFA, Università degli Studi di Bologna, Viale Berti Pichat 6/2, Bologna, Italy
J. Jasche
Affiliation:
Excellence Cluster Universe, TUM, Boltzmannstrasse 2, Garching, Germany
H. Junklewitz
Affiliation:
Argelander-Institut für Astronomie, Auf dem Hügel 71, Bonn, Germany
F. Loi
Affiliation:
DIFA, Università degli Studi di Bologna, Viale Berti Pichat 6/2, Bologna, Italy
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Abstract

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The new generation of radio interferometers will deliver an unprecedented amount of deep and high resolution observations. In this proceedings, we present recent algorithmic advances in the context of the study of cosmic magnetism in order to extract all the information contained in these data.

Keywords

magnetic fieldspolarizationmethods: numerical methods: statistical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium A30: Astronomy in Focus XXX , August 2018 , pp. 323 - 327
Copyright
© International Astronomical Union 2020

References

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