Fig. 13

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Distributions of flux density of confirmed and candidate radio halos (in blue) with 100 ≤ re ≤ 400 kpc from Botteon et al. (2022), our upper limits (in red), and upper limits from Cuciti et al. (2021a; in black), and George et al. (2021a; in yellow). Upper limits from the literature are re-scaled to 150 MHz by assuming α = 1.3. The samples are split in redshift bins as z < 0.3 (top panel) and z > 0.3 (lower panel).
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