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Table 1.

A sample of non-PSZ2 galaxy clusters that host diffuse sources in the LoTSS-DR2 fields.

No. Name RA Dec z R500 M500 Scale X-ray Ref.
[deg] [deg] [Mpc] [ × 1014 M⊙] [ × 1014 M⊙] [kpc/′]
1 Abell 84 10.4794 21.3771 0.102 0.96 ± 0.02 2.88 ± 0.43 2.86 ± 0.41 114 R A89, W15
2 Abell 373 40.8613 27.9950 0.149 – – – 157 R A89, G00
3 Abell 1213 169.1211 29.2603 0.048 – – – 57 X A89, W98
4 Abell 1330 174.5984 49.5231 0.278 1.13 5.80 (b) 5.54 253 – A89, W15
5 Abell 1889 214.1619 30.7358 0.185 0.91 ± 0.05 2.58 ± 0.39 2.58 ± 0.37 189 C(a), R A89, W15
6 Abell 1943 219.4128 30.2341 0.336 1.31 8.70 (b) 8.14 289 – A89, W15
7 Abell 1963 221.2036 31.4731 0.210 1.10 4.40 (b) 4.27 206 – S99, W15
8 DESI 201 213.3731 43.9794 0.344 0.57 ± 0.04 0.77 ± 0.16 0.82 ± 0.16 297 – Z21
9 DESI 296 138.2320 41.9373 0.155 0.55 ± 0.04 0.56 ± 0.12 0.61 ± 0.12 163 X Z21
10 MCXC J0928.6+3747 142.1570 37.7990 0.247 0.95 3.15 3.90 236 R P11
11 MCXC J0943.1+4659 145.7790 46.9980 0.406 0.97 3.97 4.75 330 X P11
12 MCXC J1020.5+3922 155.1270 39.3800 0.143 0.47 0.33 0.58 152 – P11
13 MCXC J1711.0+3941 257.7620 39.6940 0.065 0.70 1.02 1.50 76 R P11
14 PSZRX G095.27+48.27 230.8676 59.8819 0.362 – 3.23 3.34 307 – T19
15 PSZRX G100.21-30.38 350.5707 28.5264 0.388 – 5.71 5.77 320 X T19
16 PSZRX G102.17+48.88 223.7294 62.9749 0.292 – 3.13 3.25 266 – T19
17 PSZRX G116.06+80.14 194.3289 36.9139 0.518 – 6.74 6.76 378 X(a), R T19
18 PSZRX G181.53+21.43 110.3160 36.7426 0.175 – 2.28 2.40 180 R T19
19 PSZRX G195.91+62.83 162.0091 31.6423 0.515 – 5.55 5.62 378 – T19
20 WHL J002056.4+221752 5.2352 22.2977 0.199 0.60 0.86 (b) 0.96 200 R W15
21 WHL J002311.7+251510 5.7987 25.2527 0.109 0.75 1.38 (b) 1.46 121 – W15
22 WHL J085608.5+541855 134.0355 54.3152 0.251 – 2.93 (b) 2.80 238 R W15
23 WHL J091721.4+524607 139.3391 52.7685 0.192 – 4.10 (b) 3.76 194 – W15
24 WHL J101350.8+344251 153.4616 34.7142 0.146 – 2.56 (b) 2.49 155 – W15
25 WHL J130503.5+314255 196.2644 31.7153 0.396 0.90 3.52 (b) 3.29 325 – W15
26 WHL J165540.4+334422 253.9183 33.7394 0.255 0.72 1.25 (b) 1.33 241 – W15
27 WHL J172125.4+294144 260.3557 29.6957 0.184 – 2.32 (b) 2.29 187 – W15
28 WHL J173424.0+332526 263.5999 33.4239 0.485 0.60 1.26 (b) 1.34 366 – W15

Notes. Column 1: cluster number in the sample. Column 2: cluster name. Column 3: Right Ascension (J2000). Column 4: Declination (J2000). Column 5: cluster redshift. Column W15: the radius enclosing the cluster volume at which the mean over-density is 500 times the critical density of the Universe at the cluster redshift. Column 7: cluster mass within R500. Column 8: cluster mass that is scaled to that of the PSZ2 clusters (see Sec. 5.2). Column 9: angular scale at the cluster redshift. Column 10: available X-ray data. Available X-ray data is denoted as C for Chandra, X for XMM-Newton, and R for ROSAT. Column 11: reference. A89: Abell et al. (1989), G00: Gal et al. (2000), P11: Piffaretti et al. (2011), S99: Struble & Rood (1999), T19: Tarrío et al. (2019), W98: Wu et al. (1998), W15: Wen & Han (2015), Z21: Zou et al. (2021).

(a)

Proprietary data.

(b)

M500 is derived using the M500-richness scaling relation (Eq. (17) in Wen & Han 2015).

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