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. E.1.

Cosmic web structure type volume-filling fractions (VFFs) as predicted by the cubic unit cell model of Sect. 3. These VFFs depend on just one parameter: the ratio between the (comoving) filament width and the (comoving) cubic unit cell edge length .

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