VACCA, VALENTINAVALENTINAVACCAMURGIA, MATTEOMATTEOMURGIAGOVONI, FEDERICAFEDERICAGOVONIEnßlin, TorstenTorstenEnßlinOppermann, NielsNielsOppermannFERETTI, LUIGINALUIGINAFERETTIGiovannini, GabrieleGabrieleGiovanniniLOI, FRANCESCAFRANCESCALOI2020-10-292020-10-2920182075-4434http://hdl.handle.net/20.500.12386/28067The formation and history of cosmic magnetism is still widely unknown. Significant progress can be made through the study of magnetic fields properties in the large-scale structure of the Universe: galaxy clusters, filaments, and voids of the cosmic web. A powerful tool to study magnetization of these environments is represented by radio observations of diffuse synchrotron sources and background or embedded radio galaxies. To draw a detailed picture of cosmic magnetism, high-quality data of these sources need to be used in conjunction with sophisticated tools of analysis.ELETTRONICOenArticle10.3390/galaxies60401422-s2.0-85059409615000455380200043https://www.mdpi.com/2075-4434/6/4/1422018Galax...6..142VFIS/05 - ASTRONOMIA E ASTROFISICA