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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