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Table B.1.

Properties of the observed radio relics.

Name z M500c Pos. P1.4 GHz LLS Ref. Name z M500c Pos. P1.4 GHz LLS Ref.
[1014 M⊙] [1024 W Hz−1] [Mpc] [1014 M⊙] [1024 W Hz−1] [Mpc]
Abell 1656ℐ 0.023 7.17 0.31 0.85 1 PSZ G087* 0.222 3.83 0.03 1.0 15
PSZ2G146*, ℐ 0.03 1.8 0.02 0.37 2 SPT2023-5535ℐ 0.23 6.49 3.4 0.5 23,24
Abell 168 0.045 1.24 0.14 0.8 3 Abell 746 0.232 5.34 W 4.25 1.8 25
Abell 3376 0.046 3.64 E 0.54 1.6 4 N 0.18 0.38 25
W 0.40 0.96 4 E 0.19 0.95 25
Abell 3667 0.056 5.77 NW 15.1 2.3 5 PSZ2 G181* 0.240 4.23 S 0.48 1.66 15
SE 2.6 1.6 5 N 0.20 1.39 15
Abell 3266ℐ 0.059 6.64 0.24 0.58 6 RXCJ1314 0.244 6.15 W 3.90 0.91 13
CIZA J0649 0.064 3.3 1.2 0.80 7,8 E 1.68 1.13 13
ClG 0217+70 0.066 10.6 SE 0.99 3.5 9 MCXC J0929* 0.247 3.9 SW 0.3 0.30 17
SE 1.27 5.1 9 SE 0.2 0.35 17
W 1.85 2.3 9 Abell 521 0.247 7.26 SE 3.09 0.93 26
RXC J1053 0.070 1.1 0.2 0.6 7,8 ZwCl2341 0.27 5.15 S 4.09 1.23 13
Abell 1904* 0.070 1.83 N 0.32 0.23 10 N 1.82 0.57 13
S 0.005 0.17 10 Abell 1758S* 0.280 8.22 0.22 0.54 15
NE 0.01 0.9 10 SPT2023-5627 0.284 5.74 SE 1.40 0.73 27
Abell 2061 0.078 3.59 0.45 0.68 7 NW 0.91 0.86 27
Abell 2255 0.081 5.38 0.18 0.70 7 Abell 959* 0.289 5.08 0.22 0.81 15
Abell 2249 0.084 3.73 0.41 1.3 11 1E 0657-55.8 0.296 11.4 E 43.5 0.99 28
Abell 2018* 0.088 2.51 0.04 1.1 10 NNW 0.6 0.90 28
Abell 2108* 0.092 1.8 0.01 0.2 12 Abell 781 0.295 6.13 4.47 0.44 1
Abell 3365 0.093 1.7 E 0.74 0.55 13,14 PSZ2 G198* 0.299 5.5 0.51 1.49 15
W 0.09 0.29 13,14 PSZ1G097 0.3 4.7 S 3.12 1.42 13
Abell 523 0.10 1.7 1.7 1.35 7,8 N 1.52 0.88 13
ZwCl0008 0.103 3.30 E 1.54 1.41 13 Abell 1300 0.3072 8.97 5.75 0.70 1
W 0.30 0.30 13 Abell 2744 0.308 9.84 NE 4.37 1.5 29
Abell 1925* 0.105 2.81 N 0.12 1.71 15 SE 0.96 1.15 29
S 0.08 1.09 15 MACS J0258 0.322 0.39 16
Abell 2034 0.113 5.85 0.89 0.22 7 Abell 1943* 0.336 8.14 0.03 0.37 17
Abell 3186 0.127 6.44 2.5 2.0 16 PSZ2 G121* 0.344 5.69 0.21 0.54 15
WHL J1013* 0.146 2.49 0.01 0.31 17 PSZ2 G096* 0.350 5.39 0.60 1.48 15
PSZ2 G278 0.158 3.6 N 1 0.66 18 PSZRX G095* 0.362 3.34 0.8 1.30 17
S 0.7 1.64 18 PSZ2 G092* 0.362 6.31 0.32 1.53 15
Abell 1240 0.159 3.71 S 0.73 1.28 13 MACS J1752 0.366 6.96 NE 33.1 1.19 13
N 0.43 0.87 13 SW 15.0 0.69 13
Abell 3411 0.169 6.59 5.0 1.9 19 PSZ2 G114* 0.371 7.58 N 3.40 1.17 15
PSZ2 G109* 0.173 3.26 0.50 1.17 15 S 0.83 1.48 15
PSZRX G182* 0.175 2.4 0.3 1.00 17 ZwCl1447 0.376 3.4 SW 1.11 1.2 30
Abell 2345 0.177 5.92 W 2.85 0.83 13 NE 0.51 0.3 30
E 2.66 1.57 13 PSZ2 G187* 0.378 6.84 0.27 0.72 15
Abell 1612 0.179 4.42 7.9 0.78 7 PSZ1 G287 0.39 13.89 NW 23.3 2.48 13
Abell 1697*, ℐ 0.183 4.34 0.38 0.7 10 SE 9.71 1.58 13
WHL J1721* 0.184 2.29 0.08 0.60 17 WHL J1305* 0.396 3.29 0.06 1.40 17
Abell 1889* 0.185 2.58 NW 0.50 1.65 17 PSZ2 G117* 0.396 7.61 0.32 0.56 15
SE 0.40 1.65 17 MCXC J0943* 0.406 4.75 0.4 0.53 17
PSZ2 G145* 0.190 4.25 0.04 0.77 15 PSZ2 G206* 0.447 7.39 S 0.25 0.66 15
CIZAJ2243 0.192 16.2 N 15.0 2.00 13,20 N 0.18 0.66 15
S 1.95 1.65 13,20 PSZ2 G191* 0.488 5.55 2.49 0.57 15
Abell 115 0.197 7.65 2.7 2.5 21 MACS J1149 0.544 8.55 W 6.03 0.70 13
Abell 2163 0.203 16.1 2.09 0.48 1 E 5.33 0.78 13
1RXS J0603 0.22 10.76 N 65.0 1.9 22 PSZ2 G069 0.762 5.69 3.75 1.49 15
E 2.5 1.1 22 PSZ2 G092 0.822 7.4 5.25 0.9 31
S 1.4 0.25 22 ACT J0102 0.87 8.80 NW 29.6 0.93 13
PLCK G201 0.22 2.7 E 3.9 1.19 16 SE 4.48 0.46 13

Notes. Column 1: cluster name. Column 2: cluster redshift. Column 3: radio luminosity at 1.4 GHz. We derive the luminosity assuming the radio spectrum of S ∝ ν−1.5 for the radio relics only detected at a low frequency. These radio relics are annotated with *. The inverted radio relics are marked with ℐ. Column 4: largest linear size (LLS). Column 5: reference for the cluster radio luminosity.

References. (1) Feretti et al. (2012); (2) Botteon et al. (2021); (3) Dwarakanath et al. (2018); (4) Chibueze et al. (2023); (5) de Gasperin et al. (2022); (6) Riseley et al. (2022); (7) van Weeren et al. (2011b); (8) Pratt et al. (2009); (9) Hoang et al. (2021); (10) van Weeren et al. (2021); (11) Locatelli et al. (2020(; (12) Schellenberger et al. (2022); (13) de Gasperin et al. (2014(; (14) Lovisari & Reiprich (2019); (15) Botteon et al. (2022); (16) Knowles et al. (2022); (17) Hoang et al. (2022); (18) Koribalski et al. (2023(; (19) van Weeren et al. (2013); (20) Jee et al. (2015(; (21) Govoni et al. (2001a); (22) van Weeren et al. (2016); (23) HyeongHan et al. (2020); (24) Bulbul et al. (2019); (25) Rajpurohit et al. (2024); (26) Giacintucci et al. (2006); (27) Duchesne et al. (2021); (28) Sikhosana et al. (2023); (29) Pearce et al. (2017); (30) Lee et al. (2022); (31) Di Gennaro et al. (2023).

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