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Table A.2.

LoTSS GRGs in galaxy clusters.

No Cluster name GRG RA GRG Dec z r200 RL* M200 N200
(Mpc) (1014M)
1 WHL J112126.4+534457 11 21 26.44 +53 44 56.71 0.10378 ± 0.00002 1.7 69.4 4.6 46
2 WHL J113250.7+505705 11 32 50.67 +50 57 04.68 0.35857 ± 0.00010 0.9 16.9 0.9 14
3 WHL J113503.2+482612 11 35 03.20 +48 26 12.12 0.22597 ± 0.00006 1.1 21.7 1.2 17
4 WHL J121900.8+505255 12 19 00.76 +50 52 54.41 0.38509 ± 0.00008 0.9 17.3 0.9 14
5 GMBCG J188.75636+53.29864 12 35 01.52 +53 17 55.09 0.34480 ± 0.00030
6 GMBCG J191.35486+47.11948 12 45 25.16 +47 07 10.11 0.51179 ± 0.00015
7 WHL J124913.2+500044 12 49 13.20 +50 00 43.68 0.34956 ± 0.00010 1.1 25.3 1.4 30
8 WHL J125142.1+503425 12 51 42.04 +50 34 24.65 0.54904 ± 0.00007 1.1 24.3 1.4 11
9 WHL J131404.6+543938 13 14 04.60 +54 39 37.88 0.34645 ± 0.00008 1.2 26.1 1.5 23
10 WHL J132229.1+504845 13 22 29.07 +50 48 44.53 0.18439 ± 0.00004 0.9 15.9 0.8 11
11 WHL J133258.3+535356 13 32 58.28 +53 53 55.60 0.32261 ± 0.00009 0.9 16.6 0.9 13
12 WHL J133512.0+494427 13 35 12.01 +49 44 27.20 0.436 ± 0.041( † ) 0.9 14.7 0.7 9
13 WHL J133618.8+533952 13 36 18.75 +53 39 52.12 0.30138 ± 0.00006 0.9 13.4 0.7 11
14 WHL J134207.0+472553 13 42 06.98 +47 25 53.04 0.17213 ± 0.00004 0.9 13.2 0.7 13
15 WHL J142857.4+542353 14 28 57.40 +54 23 52.99 0.40573 ± 0.00011 1.2 30.7 1.8 22
16 WHL J142933.4+544336 14 29 33.45 +54 43 35.29 0.12328 ± 0.00002 1.3 34.7 2.0 29
17 WHL J144410.5+554746 14 44 10.50 +55 47 45.64 0.33475 ± 0.00005 1.2 30.1 1.7 26
18 WHL J144520.9+540330 14 45 20.87 +54 03 29.62 0.43345 ± 0.00013 1.0 25.1 1.4 18
19 GMBCG J222.81919+51.22588 14 51 16.59 +51 13 33.28 0.509 ± 0.050( † )
20 WHL J150624.1+535503 15 06 24.10 +53 55 02.61 0.30437 ± 0.00005 1.0 19.1 1.0 11

Notes. Parameters r200 and RL* (cluster richness parameter) have been taken from the WHL galaxy cluster catalogue and M200 was computed from Eq. (2) of Wen et al. (2012). GRGs marked with ( † ) in the redshift column have photometric redshift estimate and the rest have spectroscopic redshifts. r200 is the radius within which the mean density of a cluster is 200 times of the critical density of the Universe, and M200, is the mass of the cluster within r200. N200 is the number of galaxies within r200. Clusters 6, 7, and 20 are identified from GMBCG cluster catalogue (Hao et al. 2010).

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