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. 11.

Merger- and accretion-shocked synchrotron Cosmic Web (MASSCW) specific intensity prior marginal medians at observing frequency ν_obs = 150 MHz for three deep LOFAR HBA fields. Individual shocks should not be discernible in these statistical aggregates. The colour scales share the same lower bound. Top: Lockman Hole. Middle: Abell 2255. Bottom: Ursa Major Supercluster.

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