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

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Vacca,  V.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons16142

Enßlin,  T.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons37994

Selig,  M.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Greiner,  M.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons16134

Reinecke,  M.
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Vacca, V., Oppermann, N., Enßlin, T., Jasche, J., Selig, M., Greiner, M., et al. (2016). Using rotation measure grids to detect cosmological magnetic fields: A Bayesian approach. Astronomy & Astrophysics, 591: A13, pp. 1-22. doi:10.1051/0004-6361/201527291.


Cite as: http://hdl.handle.net/11858/00-001M-0000-002B-1BB5-E
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