Published March 8, 2018
| Version v1
Dataset
Open
The primordial magetic field in the local Universe
Authors/Creators
- 1. Max Planck Institute for Astrophysics, Karl-Schwarzschildstr.1, 85741 Garching, Germany
- 2. Department of Physics, Stockholm University, Albanova University Center, SE 106 91 Stockholm, Sweden
- 3. University of Bologna, Department of Physics and Astronomy, Via Gobetti 93/2, I-40129, Bologna, Italy
- 4. Sorbonne Université & CNRS, UMR 7095, Institut d'Astrophysique de Paris, 98 bis bd Arago, 75014 Paris, France
- 5. INAF/OAS Bologna, Via Gobetti 101, I-40129 Bologna, Italy
Description
This dataset contains the 3D structure of large scale magnetic fields in the local Universe, which were seeded by density perturbations during the radiation dominated epoch and later on were evolved by structure formation. This relies on three dimensional initial density fields inferred from the 2M++ galaxy compilation via the Bayesian algorithm. Using those, we estimate the magnetogenesis by the so called Harrison mechanism.