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Table 1.

Summary of sample of galaxy clusters used in this paper.

Cluster name RA (J2000) Dec (J2000) z cSB M500 STGSS SVLASS SLoTSS
(1014M) (mJy) (mJy) (mJy)
RCS 1419+5326 14h19m12.1s 53d26m11.6s 0.620 0.185 2.60 (2)
CDGS40 14h50m09.0s 09d04m48.7s 0.644 0.103 1.86 (4) ...
EGSXG J1417.9+5235 14h17m53.7s 52d34m46.2s 0.683 0.119 0.55 (4)
EGSXG J1420.5+5308 14h20m33.3s 53d08m21.1s 0.734 0.160 1.07 (4) 92 11 81
MS 1137+6625 11h40m22.8s 66d08m14.5s 0.782 0.096 4.70 (4)
RX J1317+2911 13h17m21.8s 29d11m17.0s 0.805 0.123 1.73 (4)
RX J1716+6708 17h16m38.8s 67d08m25.8s 0.813 0.082 5.10 (1) 2.5 51
EGSXG J1416.2+5205 14h16m16.7s 52d05m58.2s 0.832 0.120 1.31 (4) 2.6 17
RX J1226+3333 12h26m58.2s 33d32m48.0s 0.890 0.083 7.80 (3) 1.9 28
CDGS54 10h02m01.0s 02d13m28.6s 0.900 0.093 2.32 (4) 19.2 3.9 ...
CL J1415+3612 14h15m11.2s 36d12m04.0s 1.030 0.151 3.44 (4) 2.9 7.0
RX J0910+5422 09h10m45.4s 54d22m05.0s 1.106 0.101 0.87 (4) 2.0
RX J0849+4452 08h28m58.2s 44d51m55.1s 1.261 0.099 2.84 (4)

Notes. High-resolution LOFAR observations have been processed for the galaxy clusters indicated with boldface. The total flux density of each source is listed as reported by three radio surveys: TGSS at 150 MHz, VLASS at 3 GHz, and LoTSS at 144 MHz. Non-detections are indicated with a horizontal dash. Sources located beyond the coverage of the corresponding survey are indicated with ellipsis.

References. (1) Ettori et al. (2004); (2) Hicks et al. (2008); (3) Mantz et al. (2010); (4) Pascut & Ponman (2015).

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