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Table 4

Properties of the diffuse cluster sources in the GMRT radio Halo survey.

Cluster name Radio source ν Sν Pν LLS HPBW
(MHz) (mJy) W HZ-1 (Mpc) ()
A 2744 GRH 325 323 ± 26 9.68 × 1025 ~1.9 35.0 × 35.0
Rel 325 122 ± 10 3.66 × 1025 ~1.3 35.0 × 35.0
A 209 GRH 325 74 ± 6a 8.91× 1024 ~0.6a 25.0 × 25.0
A 1300 GRH 325 130 ± 10 3.92 × 1025 ~0.9 28.0 × 28.0
Rel 325 75 ± 6 2.26 × 1025 ~0.5 28.0 × 28.0
Cand. Rel 325 23 ± 2 6.94 × 1024 ~0.7 28.0 × 28.0
A 1682 Diffuse Comp. 240 46 ± 4 6.82× 1024 ~0.3 18.3 × 14.0
RXCJ 1314.4–2515 W Rel 325 137 ± 11 2.42 × 1025 26.1 × 10.2
E Rel 325 52 ± 4 9.18 × 1024 26.1 × 10.2
RH 325 40 ± 3 7.06 × 1024 26.1 × 10.2
A 1758N GRH 325 155 ± 12 3.75 × 1025 ~1.5 35.0 × 35.0
A 521b GRH 240 152 ± 15 2.79 × 1025 ~0.9 35.0 × 35.0
A 521b Rel 240 180 ± 10 3.30 × 1025 ~1 35.0 × 35.0
A 521c Rel 325 114 ± 6 2.09 × 1025 ~1 16.0 × 13.0
A 697d GRH 325 47.3 ± 2.7 1.16 × 1025 ~1.3 46.8 × 41.4
A 781e Rel 325 93.3 ± 7.5 2.61 × 1025 ~0.8 40.0 × 37.0
RXCJ 2003.5–2323f GRH 240 360 ± 18 1.16× 1026 ~1.4 35.0 × 35.0

Notes.

(a)

The value should be considered a lower limit, see Sect. 3.1.1.

(b)

Information taken from Brunetti et al. (2008).

(c)

Information taken from Giacintucci et al. (2008).

(d)

Information taken from Macario et al. (2010).

(e)

Information taken from Venturi et al. (2011a).

(f)

Information taken from Giacintucci et al. (2009).

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