Table 1
Sample of sources extracted from the LOFAR Deep Fields.
| Source name | Field | Redshift | M500 (1014 M⊙) | R500 (Mpc) | Radio classification |
|---|---|---|---|---|---|
| MCXC J1033.8+5703 | Lockman | 0.0463 | 0.128 | 0.35 | No detection |
| MCXC J1036.1+5713 | Lockman | 0.7699 | 3.25 | 0.78 | Halo |
| MCXC J1053.3+5720 | Lockman | 0.34 | 0.487 | 0.49 | No detection |
| PSZ2 G147.88+53.24 | Lockman | 0.60 | 6.47 ± 0.60 | 1.06 | Halo |
| PSZ2 G149.22+54.18 | Lockman | 0.1369 |  |
1.22 | Halo |
| SpARCS1049+56 | Lockman | 1.71(1) | 2.52 ± 0.86(2) | 0.51 | AGN |
| SDSSC4-3094 | Lockman | 0.04632(3) | AGN | ||
| PSZRX G084.01+46.28 | ELAIS-N1 | 0.0675 |  |
0.77 | No detection |
| PSZ2 G084.69+42.28 | ELAIS-N1 | 0.13 |  |
0.94 | Uncertain |
| WHL J160439.5+543139 | ELAIS-N1 | 0.2655 | 2.95 ± 0.50 | 0.93 | Detection uncertain |
| WHL J161135.9+541635 | ELAIS-N1 | 0.3407 | 3.40 ± 0.58 | 0.94 | No detection |
| WHL J161420.1+544254 | ELAIS-N1 | 0.3273 | 2.85 ± 0.48 | 0.89 | Detection uncertain |
Notes. The mass, redshift and R500 are obtained from the PSZ2 catalogue (Planck Collaboration XXVII 2016) or from the MCXC catalogue (Piffaretti et al. 2011)if the source was not present in the former catalogue, unless otherwise noted. For the WHL clusters M500 was estimated from the richness, as detailed in Sect. 5.7. Mass uncertainties are not available for MCXC clusters.
References. (1) Webb et al. (2015). (2) Derived from M200 given in Finner et al. (2020), see Sect. 5.5. (3)Miller et al. (2005).
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