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    Radio Observations as a Probe of Cosmic Web Magnetism by Ettore Carretti, Franco Vazza

    Published 2025-05-01
    “…Independently of the scenario and the shape of the astrophysical component RM, it is in the range 10–60 nG at <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mi>z</mi><mo>=</mo><mn>0</mn></mrow></semantics></math></inline-formula>, while, when restricted to the model that gives the best match to the simulations, it gives <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mn>43</mn><mo>±</mo><mn>7</mn></mrow></semantics></math></inline-formula> nG, with an astrophysical component RM rapidly decreasing with the redshift.…”
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