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Table 3.

Cluster radio properties.

Cluster Classification LLS S144
(Mpc) (mJy)
PSZ2 G080.16+57.65 cHalo, Relic (R) 1.1, (H) ∼1 (H) 92 ± 32, (R) 55.8 ± 11.6
PSZ2 G084.10+58.72(a) cHalo 0.5 4.2 ± 1.2
PSZ2 G086.93+53.18(a) Halo 0.6 12.4 ± 3.6
PSZ2 G087.39+50.92 AGN-no diffuse
PSZ2 G088.98+55.07 AGN-no diffuse
PSZ2 G089.52+62.34 (A) Relic (A) 0.23 (A+C) 74.6 ± 15.0
(B) cRelic (A+B: cdRelic) (B) 0.17 (B) 12.2 ± 2.6
D (Relic) (D) 0.9 (D) 31.8 ± 8.2
PSZ2 G095.22+67.41 cRelic 0.4 6.8 ± 1.5
PSZ2 G096.14+56.24 AGN-no diffuse
PSZ2 G098.44+56.59 AGN-no diffuse
PSZ2 G099.86+58.45(b) Halo 1.0 14.7 ± 3.2
PSZ2 G106.61+66.71 cHalo 0.5 20 ± 4
PSZ2 G107.10+65.32(c) dHalo (Hn) 2.0, (Hs) 1.3 (Hn) 123 ± 25, (Hs) 63 ± 14
Relic (s) 0.5 20.9 ± 4.3
cFossil (n: S1, S2) (S1) 0.4, (S2) 0.23 (S1) 79 ± 17, (S2) 17.5 ± 3.6
PSZ2 G111.75+70.37(d) Relic 0.7 (R) 106.7 ± 21.4
Halo ∼0.6 27.7 ± 6.3
PSZ2 G114.31+64.89 Halo 0.5 91.7 ± 18.6
PSZ2 G114.99+70.36(e) cHalo, cFossil ( ⋆ )
PSZ2 G118.34+68.79 cHalo, Fossil (H) ∼0.4, (F) 0.5 (H) 28 ± 13, (F) 67 ± 13
PSZ2 G123.66+67.25 cFossil 0.26 7.5 ± 1.6
PSZ2 G133.60+69.04(f) Halo, cdRelic/cFossil (H) 0.9 (H) 129 ± 26
PSZ2 G135.17+65.43 cHalo 0.5 29.0 ± 6.6
cRelic/cFossil 0.4 9.14 ± 1.9
PSZ2 G136.92+59.46 AGN-no diffuse
PSZ2 G143.26+65.24(g) Halo 1.5 (H) 29.8 ± 6.6
PSZ2 G144.33+62.85 AGN-no diffuse
PSZ2 G145.65+59.30 cHalo/cFossil 0.4 6.7 ± 1.7
PSZ2 G150.56+58.32 Halo 1.0 71.2 ± 14.5
PSZ2 G151.62+54.78 AGN-no diffuse
PSZ2 G156.26+59.64 cHalo 0.5 7.9 ± 3.7

RXC J1053.7+5452(h) Relic 0.75 214 ± 43
Abell 1156 cHalo 0.7 15.7 ± 6.8
Abell 1314(i) Fossil (central) 0.44 136.9 ± 27.4
Abell 1615 AGN-no diffuse
MaxBCG J173.04772+47.81041 AGN-no diffuse
NSC J143825+463744 Unclassified 0.4
GMBCG J211.77332+55.09968 AGN-no diffuse
WHL J125836.8+440111 Halo 0.8 58.4 ± 11.7
WHL J122418.6+490549 Fossil 0.37 209 ± 42
WHL J124143.1+490510 cHalo 1.2 ( ⋆ )
WHL J132226.8+464630 cHalo 0.5 ( ⋆ )
WHL J132615.8+485229 AGN-no diffuse 0.32 ( ⋆ )
WHL J133936.0+484859 cHalo ∼0.3 ( ⋆ )
WHL J134746.8+475214 AGN-no diffuse

Notes. H = halo, R = relic, d = double, c = candidate, s = south, n = north, LLS = largest linear size. ( ⋆ )Radio emission is blended with other sources, and therefore no reliable flux density measurement can be obtained. Literature references that first reported the presence of diffuse emission in these clusters: (a)Di Gennaro et al. (2021); (b)Cassano et al. (2019); (c)Kempner & Sarazin (2001) and Botteon et al. (2018); (d)Shimwell et al. (2019); (e)Venturi et al. (2008); (f)Govoni et al. (2012); (g)Hoeft et al. (2020); (h)Rudnick & Lemmerman (2009); (i)Wilber et al. (2019).

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