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Table 9

Radio halo sample clusters.

Name z kpc/" S (1.4) ΔS log P(1.4) LLS Luminosity Temperature Exposure time Ref.
mJy mJy W/Hz Mpc (1044 erg/s) (keV) ks

A1914 0.1712 2.80 64.0 3.0 24.04 1.01 9.86 10.50 19 1, 2
A2218 0.1756 2.86 4.7 0.1 22.96 0.37 5.46 6.70 59 1, 2
A665 0.1819 2.95 43.1 2.2 23.92 1.77 9.13 8.30 39 1, 2
A520 0.1990 3.16 34.4 1.5 23.91 1.08 7.85 7.40 9 1, 2
A773 0.2170 3.38 12.7 1.3 23.57 1.21 7.52 8.53 20 1, 2
IE0657-56 0.2960 4.26 78.0 5.0 24.64 2.0 21.37 11.64 84 1, 2
A2255 0.0806 1.46 56.0 3.0 23.28 0.8 2.50 6.42 39 1, 2
A2319 0.0557 1.04 153.0 8.0 23.38 1.0 8.00 9.49 14 1, 2
A754 0.0542 1.01 86.0 4.0 23.12 0.96 2.10 9.94 44 1, 2
A2256 0.0581 1.08 103.4 1.1 23.26 0.79 3.55 6.90 12 1, 2
A401 0.0737 1.34 17.0 1.0 22.70 0.50 6.17 8.07 18 1, 2
A3562 0.0490 0.92 20.0 2.0 22.41 0.27 1.48 3.80 19 1, 2
A399 0.0718 1.31 16.0 0 22.67 0.55 3.60 5.80 48 3, 2
A2163 0.2030 3.22 155.0 2.0 24.57 2.21 21.50 12.12 71 1, 2
A1300 0.3072 4.37 20.0 2.0 24.10 1.26 13.0 9.2 14 1, 4
A1758 0.2790 4.08 16.7 0.8 23.93 1.47 6.70 7.95 7 1, 2
A1995 0.3186 4.48 4.1 0.7 23.47 0.80 8.35 8.60 56 1, 2
A2034 0.1130 1.97 13.6 1.0 23.00 0.59 3.60 7.15 195 1, 2
A209 0.2060 3.25 16.9 1.0 23.65 1.36 5.84 8.28 20 1, 2
A2219 0.2256 3.48 81.0 4.0 24.40 1.67 11.53 9.81 42 1, 2
A2294 0.1780 2.90 5.8 0.5 23.06 0.52 3.70 7.10 10 1, 2
A2744 0.3080 4.38 57.1 2.9 24.55 1.84 12.16 9.61 24 1, 2
A521 0.2533 3.80 5.9 0.5 23.40 1.14 8.01 6.74 37 1, 2
A697 0.2820 4.11 7.8 1.0 23.62 0.63 9.84 9.06 27 1, 2
RXCJ2003.5-2323 0.3171 4.46 35.0 2.0 24.40 1.36 8.63 9.1 50 1, 5

Notes. Columns: (1) cluster name; (2) redshift; (3) conversion factor (angular size to linear size); (4) radio flux density (1.4 GHz); (5) error in estimated radio flux density; (6) total radio power (1.4 GHz); (7) radio largest linear size; (8) total X-ray luminosity (0.12.4 keV); (9) temperature (keV); (10) exposure time; (11) references. We normalised H dependent quantities with H0 = 73 km s-1 Mpc-1.

Reference. 1 = Giovannini et al. (2009, and references therein); 2 = Cavagnolo et al. (2009); 3 = Feretti et al. (2012, and references therein); 4 = Ziparo et al. (2012); 5 = Giacintucci et al. (2009).

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