The topology of the magnetic field in Abell 2255 out to its virial radius. Results from the LOFAR Galaxy Cluster Ultra-Deep Field
A. Botteon, R. J. van Weeren, Y. Hu, F. Vazza, G. Brunetti, K. Rajpurohit, A. Lazarian, T. W. Shimwell, E. De Rubeis, M. Balboni, A. Bonafede, R. Cassano, G. Di Gennaro, F. Gastaldello, M. J. Hardcastle, A. Ignesti, H. J. A. Röttgering
astro-ph.CO, astro-ph.GA, astro-ph.HE
Submitted: 2026-07-15
Comments: 15 pages, 10 figures + Appendix. Accepted for publication in A&A
Code: https://github.com/lofar-astron/prefactor
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Anticipated Performance of the Square Kilometre Array -- Phase 1 (SKA1)
- The Pan-STARRS1 Surveys
- Applying Wirtinger derivatives to the radio interferometry calibration problem
Related papers
- Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
- A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
- Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
- Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
- Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation