T
Torsten A. Ensslin
Researcher at Max Planck Society
Publications - 80
Citations - 20738
Torsten A. Ensslin is an academic researcher from Max Planck Society. The author has contributed to research in topics: Galaxy & Galaxy cluster. The author has an hindex of 41, co-authored 80 publications receiving 19932 citations. Previous affiliations of Torsten A. Ensslin include University of Toronto.
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Using rotation measure grids to detect cosmological magnetic fields -- a Bayesian approach
V. Vacca,Niels Oppermann,Torsten A. Ensslin,Jens Jasche,Marco Selig,M. Greiner,H. Junklewitz,Martin Reinecke,M. Brueggen,E. Carretti,Luigina Feretti,Chiara Ferrari,Christopher A. Hales,Cathy Horellou,S. Ideguchi,Melanie Johnston-Hollitt,Roberto Pizzo,Huub Roettgering,Timothy W. Shimwell,Keitaro Takahashi +19 more
TL;DR: In this article, a Bayesian algorithm was developed to distinguish statistically Faraday depth variance contributions intrinsic to the source from those due to the medium between the source and the observer, where the foreground and measurement noise were taken into account as the uncertainty correlations of the galactic model.
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Pacman (I): A new Algorithm to calculate Faraday Rotation Maps
TL;DR: Pacman as mentioned in this paper solves the n-pi ambiguity problem for a high signal-to-noise region ''democratically'' and uses this information to assist computations in adjacent low-signal-tonoise areas.
Posted Content
Radio observations of the Galactic Centre and the Coma cluster as a probe of light dark matter self-annihilations and decay
TL;DR: In this article, the authors predict the synchrotron spectrum as well as the morphology of the radio emission associated with light decaying and annihilating dark matter candidates in both the Coma cluster and the Galactic Centre.
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3C 129 at 90cm: Evidence for a Radio Relic?
TL;DR: In this article, the authors presented a wide-field map of the radio galaxy 3C 129 and its companion galaxy 3c 129.1 at lambda=90 cm, showing a distinct steep-spectrum feature near the head of 3C129, extending in a direction perpendicular to the radio tails.