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Table 1.
Flux densities of the cluster-scale diffuse radio emission at 144 MHz. Radio powers are calculated assuming a spectral index α = −1.5 ± 0.3 (Di Gennaro et al. 2021a,b).
| Cluster name | Redshift | LLS | 144 MHz flux density | 150 MHz radio power | 1.4 GHz radio power |
|---|---|---|---|---|---|
| z | [kpc] | S144 MHz, diff [mJy] | P150 MHz [×1025 W Hz−1] | P1.4 GHz [×1023 W Hz−1] | |
| MOOJ0123+2545 | 1.229 ( † ) | 420 | 2.1 ± 0.6 | 2.6 ± 1.1 | 9.8 ± 5.6 |
| MOOJ1231+6533 | 0.99 | 430 | 1.0 ± 0.3 | 0.7 ± 0.2 | 2.8 ± 1.3 |
| MOOJ1246+4642 | 0.90 | 390 | 1.3 ± 0.6 | 0.7 ± 0.4 | 2.8 ± 2.1 |
| MOOJ1420+3150 | 1.34 | 475 | 1.8 ± 0.8 | 2.9 ± 1.6 | 10.8 ± 6.7 |
| MOOJ2354+3507 | 0.97 | 360 | 1.6 ± 0.8 | 1.1 ± 0.5 | 4.3 ± 3.2 |
Notes. ( † )Spectroscopic redshift.
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