We use rotation measures data from the NVSS catalogue to derive new, statistically robust, upper limits on the strength of extragalactic magnetic fields. The extragalactic contribution to the rotation measures for a given field strength and correlation length grows with the distance. Based on the observation that low-luminosity distant radio sources do not exhibit any trend with their redshift, we then constrain extragalactic fields with Mpc coherence length to be below approximately 1.5 nG; a field coherent across the entire observable Universe instead is bounded to be below 0.6 nG. These limits do not depend on the particular origin of these cosmological fields.SCOPUS: cp.pinfo:eu-repo/semantics/publishe
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation pro...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society,...
We take advantage of the wealth of rotation measures data contained in the NRAO VLA Sky Survey catal...
Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation pro...
Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation pro...
Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation pro...
International audienceMeasuring the properties of extragalactic magnetic fields through the effect o...
International audienceMeasuring the properties of extragalactic magnetic fields through the effect o...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
I introduce you to the very best limits on cosmological magnetic fields. The numbers: magnetic field...
Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation pro...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation pro...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society,...
We take advantage of the wealth of rotation measures data contained in the NRAO VLA Sky Survey catal...
Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation pro...
Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation pro...
Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation pro...
International audienceMeasuring the properties of extragalactic magnetic fields through the effect o...
International audienceMeasuring the properties of extragalactic magnetic fields through the effect o...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
I introduce you to the very best limits on cosmological magnetic fields. The numbers: magnetic field...
Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation pro...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation pro...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society,...