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Table 4.
Literature sample for P150 MHz scaling relations.
| Cluster | Alternative name | Redshift | Flux density | Frequency | Reference |
|---|---|---|---|---|---|
| (mJy) | (MHz) | ||||
| PSZ2 G108.17−11.56 | PSZ1 G108.18−11.53 | 0.336 | 124 ± 11 | 147 | de Gasperin et al. (2015) |
| PSZ2 G057.80+88.00 | Coma Cluster | 0.0231 | 7200 ± 800 | 150 | Cordey (1985) |
| PSZ2 G149.22+54.18 | Abell 1132 | 0.1351 | 178 ± 27 | 144 | Wilber et al. (2018) |
| PSZ2 G058.29+18.55 | RXC J1825.3+3026 | 0.065 | 163 ± 47 | 144 | Botteon et al. (2019) |
| PSZ2 G151.19+48.27 | Abell 959 | 0.2894 | 94 ± 14 | 143 | Bîrzan et al. (2019) |
| PSZ2 G071.39+59.54 | RXC J1501.3+4220 | 0.2917 | 20.2 ± 2.0 | 144 | Wilber et al. (2019) |
| PSZ2 G139.62+24.18 | PSZ1 G139.61+24.20 | 0.2671 | 30 ± 4 | 144 | Savini et al. (2018) |
| PSZ2 G049.22+30.87 | RX J1720.1+2638 | 0.164 | 165 ± 25 | 144 | Savini et al. (2019) |
| PSZ2 G138.32-39.82 | RXC J0142.0+2131 | 0.280 | 32 ± 6 | 144 | Savini et al. (2019) |
| PSZ2 G226.18+76.79 | Abell 1413 | 0.143 | 40 ± 7 | 144 | Savini et al. (2019) |
| PSZ2 G055.59+31.85 | Abell 2261 | 0.224 | 165 ± 25 (a) | 144 | Savini et al. (2019) |
| PSZ2 G180.25+21.03 | MACS J0717.5+3745 | 0.546 | 370 ± 60 | 147 | Bonafede et al. (2018) |
| PSZ2 G195.75−24.32 | Abell 520 | 0.201 | 229.7 ± 34.8 | 145 | Hoang et al. (2019a) |
| PSZ2 G100.14+41.67 | Abell 2146 | 0.232 | 19.8 ± 5.0 (b) | 144 | Hoang et al. (2019b) |
| PSZ2 G186.37+37.26 | Abell 697 | 0.282 | 135 ± 27 | 153 | Macario et al. (2013) |
| PSZ2 G208.80−30.67 | Abell 521 | 0.247 | 328 ± 66 | 153 | Macario et al. (2013) |
| PSZ2 G008.94−81.22 | Abell 2744 | 0.308 | 415 ± 42 | 150 | George et al. (2017) |
| PSZ2 G175.69−85.98 | Abell 141 | 0.230 | 110 ± 11 | 168 | Duchesne et al. (2021) |
Notes.
(b)
A range of flux densities was provided for the radio halo by Hoang et al. (2019b). We adopted the average value of that range, with the uncertainty reflecting the provided range.
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