Filamentary baryons and where to find them - A forecast of synchrotron radiation from merger and accretion shocks in the local Cosmic Web

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Fig. A.3.

Thermal bremsstrahlung specific intensity prior marginal medians at E_obs = 1 keV for three deep LOFAR HBA fields. For merger and accretion shock synchrotron predictions of the same regions, see Fig. 11. Top: Lockman Hole. Middle: Abell 2255. Bottom: Ursa Major Supercluster.

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