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. 8.

Realisation of the merger- and accretion-shocked synchrotron Cosmic Web (MASSCW) priors at observing frequency ν_obs = 150 MHz. We show exactly 1/4 of the total sky. Top: specific intensity I_ν. Bottom: specific-intensity–weighted mean (cosmological) redshift .

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