Fig. 11
RHLF of halos with νs ≥ 120 MHz (black solid lines) and that of halos with νs > 1000 MHz (red lower lines) in two different redshift ranges z = 0.1−0.2 (left panel) and z = 0.3−0.4 (right panel). As an example, dashed lines (in both panels) show the individual contributions of “turbulent” radio halos and “off-state” halos to the LOFAR RHLF. The black and red arrows show the LOFAR and EMU+WODAN sensitivities, respectively, at the considered redshifts.
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