Table B.1.
Properties of the initial sample of PSZ galaxy clusters
| PSZ2 Name | Abell Name | z | Mass | Included | Reason for exclusion |
|---|---|---|---|---|---|
| [1014 M⊙] | |||||
| PSZ2G080.16+57.65 | A2018 | 0.0878 | 2.51 ± 0.21 | No | Halo emission mixed with old plasma |
| PSZ2G080.70+48.31 | A2136 | 0.235 | 3.20 ± 0.41 | No | Small-scale emission (mini-halo?) |
| PSZ2G081.02+50.57 | / | 0.501 | 4.69 ± 0.54 | No | Complex source subtraction |
| PSZ2G084.10+58.72 | / | 0.731 | 5.40 ± 0.62 | No | High redshift |
| PSZ2G086.93+53.18 | / | 0.6752 | 5.45 ± 0.51 | Yes | / |
| PSZ2G096.83+52.49 | A1995 | 0.318 | 4.92 ± 0.37 | Yes | / |
| PSZ2G099.86+58.45 | / | 0.616 | 6.85 ± 0.49 | Yes | / |
| PSZ2G106.61+66.71 | / | 0.3314 | 4.67 ± 0.56 | No | Complex source subtraction |
| PSZ2G107.10+65.32N | A1758N | 0.2799 | 8.00 ± 0.50 | Yes | / |
| PSZ2G107.10+65.32S | A1758S | 0.2799 | 5.10 ± 0.40 | Yes | / |
| PSZ2G111.75+70.37 | A1697 | 0.183 | 4.34 ± 0.33 | Yes | / |
| PSZ2G112.48+56.99 | A1767 | 0.070 | 2.99 ± 0.15 | No | Complex source subtraction |
| PSZ2G114.31+64.89 | A1703 | 0.2836 | 6.76 ± 0.37 | Yes | / |
| PSZ2G118.34+68.79 | / | 0.2549 | 3.77 ± 0.49 | No | Complex source subtraction |
| PSZ2G133.60+69.04 | A1550 | 0.254 | 5.88 ± 0.40 | Yes | / |
| PSZ2G135.17+65.43 | / | 0.5436 | 6.01 ± 0.60 | Yes | / |
| PSZ2G139.18+56.37 | A1351 | 0.322 | 6.87 ± 0.38 | Yes | / |
| PSZ2G143.26+65.24 | A1430 | 0.3634 | 7.65 ± 0.43 | Yes | / |
| PSZ2G150.56+58.32 | / | 0.466 | 7.55 ± 0.51 | No | Complex source subtraction |
| PSZ2G156.26+59.64 | / | 0.6175 | 6.77 ± 0.60 | No | Complex source subtraction |
Notes. The table lists our initial sample of PSZ2 galaxy clusters hosting either confirmed or candidate radio halos, following the classification of (Botteon et al. 2022), together with their Abell name, redshift and mass. The last two columns report whether the cluster was included in the final sample and, if not, the main reason for the exclusion.
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