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This article has an erratum: [https://doi.org/10.1051/0004-6361/202555587e]


Table 1.

List of the galaxy clusters in the MGCLS that host a radio halo.

Cluster name RA Dec z LAS LLS rms Beam
[deg] [deg] [arcmin] [Mpc] [μJy beam−1] [″ × ″]
Abell 85(†) 10.453 –9.318 0.056 4.0 0.26 3.3 7.7 × 7.6
Abell 209 22.990 –13.576 0.209 7.9 1.62 3.6 7.8 × 7.7
Abell 521 74.536 –10.244 0.248 5.3 1.23 3.4 8.5 × 7.9
Abell 545b 83.102 –11.543 0.154 4.7 0.75 3.1 8.3 × 8.0
Abell 2667(†) 357.920 –26.084 0.232 4.6 1.02 2.7 7.6 × 7.5
Abell 2744 3.567 –30.383 0.307 7.5 2.04 2.9 7.1 × 7.1
Abell 2811 10.537 –28.536 0.108 5.2 0.62 2.6 9.2 × 8.3
Abell 3558 201.978 –31.492 0.048 4.5 0.25 2.9 7.4 × 7.2
Abell 3562 202.783 –31.673 0.050 11.5 0.67 3.3 7.3 × 7.2
Abell S295 41.400 –53.038 0.300 4.0 1.07 2.3 8.1 × 7.9
Abell S1063 342.181 –44.529 0.348 5.5 1.62 2.6 7.1 × 7.0
Bullet Cluster 104.658 –55.950 0.297 8.5 2.26 2.8 7.9 × 7.6
El Gordo 15.719 –49.250 0.870 3.3 1.53 1.5 7.2 × 6.6
MACS J0417.5–1154(†) 64.394 –11.909 0.443 4.9 1.68 2.9 7.9 × 7.8
RXC J1314.4–2525 198.599 –25.256 0.244 4.7 1.08 4.2 7.5 × 7.4
J0145.0–5300 (Abell 2941) 26.260 –53.014 0.117 4.9 0.62 2.6 7.5 × 7.4
J0225.9–4154 (Abell 3017) 36.478 –41.910 0.220 2.4 0.51 2.7 7.6 × 7.4
J0232.2–4420 (PSZ2 G259.98–63.43) 38.070 –44.348 0.286 5.8 1.49 2.6 7.5 × 7.3
J0303.7–7752 (PSZ1 G294.68–37.01) 45.943 –77.869 0.274 3.8 0.95 2.9 7.5 × 7.5
J0352.4–7401 (Abell 3186) 59.123 –74.031 0.127 10.7 1.46 2.6 7.8 × 7.6
J0516.6–5430 (Abell S520) 79.158 –54.514 0.295 5.7 1.51 3.1 7.7 × 7.4
J0528.9–3927 (Abell 3343) 82.235 –39.463 0.284 4.0 1.06 2.6 7.3 × 7.3
J0638.7–5358 (Abell S592)(†) 99.694 –53.972 0.227 6.4 1.40 3.4 7.3 × 7.2
J0645.4–5413 (Abell 3404) 101.372 –54.219 0.164 7.7 1.30 3.4 7.7 × 7.6
J1601.7–7544 (PSZ2 G313.88–17.11) 240.445 –75.746 0.153 5.9 0.94 3.7 8.5 × 7.8
J2023.4–5535 (PSZ1 G342.33–34.92) 305.852 –55.592 0.232 4.7 1.04 2.7 7.5 × 7.5

Notes. Elongated halos and halos with embedded bright AGN sources are indicated with a dagger symbol. All values are from Knowles et al. (2022). Abell 85 is included in the list because it hosts a type of diffuse emission bridging both halo and mini-halo classifications (see Knowles et al. 2022). Column 1: cluster name; Cols. 2 and 3: coordinates; Col. 4: redshift; Col. 5: largest angular size; Col. 6: largest linear size; Cols. 7 and 8: noise and resolution of the MeerKAT image.

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