Table 5.
Flux measurements for the sample of the BCGs. The information on the observations (e.g. beam and literature references) are provided in Tables 2 and 3.
| Radio | Cluster | Telescope | ν | Stot | Scentral | Sdiff | Ref. |
|---|---|---|---|---|---|---|---|
| galaxy | name | (MHz) | (mJy) | (mJy) | (mJy) | ||
| J 1254-2900 | A 3528 N | GMRT | 235 | 996.1 ± 79.7 | This work | ||
| GMRT | 610 | 428.1 ± 21.4 | This work | ||||
| ATCA | 1380 | 230.9 ± 6.9 | (Venturi et al. 2001) | ||||
| ATCA | 2380 | 142.4 ± 4.3 | (Venturi et al. 2001) | ||||
| VLA | 8400 | 50.5 ± 1.5 | This work | ||||
| J 1254-2913 | A 3528 S | GMRT | 150 | 14491.0 ± 2898.2 | TGSS image | ||
| GMRT | 235 | 7291.4 ± 583.3 | 4714.5 ± 377.2 | 2576.9 ± 694.6 | This work | ||
| GMRT | 610 | 2159.1 ± 108.0 | 1956.7 ± 97.8 | 202.4 ± 145.8 | This work | ||
| MOST | 843 | 1970.0 ± 59.1 | SUMSS image | ||||
| ATCA | 1380 | 936.7 ± 28.1 | (Venturi et al. 2001) | ||||
| VLA | 1400 | 1069.1 ± 32.1 | 132.4 ± 42.6a | NVSS image | |||
| ATCA | 2380 | 538.4 ± 16.2 | (Venturi et al. 2001) | ||||
| VLA | 8400 | 125.3 ± 3.8 | This work | ||||
| J 1257-3021 | A 3532 | GMRT | 150 | 8655.9 ± 1410.1 | 6802.4 ± 1360.5 | 1853.5 ± 370.7 | TGSS image |
| GMRT | 235 | 4591.9 ± 336.0 | 4251.3 ± 334.9 | 340.5 ± 27.2 | This work | ||
| GMRT | 610 | 1522.0 ± 74.2 | 1484.0 ± 74.2 | 38.0 ± 1.9 | This work | ||
| MOST | 840 | 1773.0 ± 53.2 | SUMSS image | ||||
| ATCA | 1380 | 1056.5 ± 31.7 | (Venturi et al. 2001) | ||||
| VLA | 1400 | 1061.0 ± 31.8 | 4.5 ± 44.4a a | NVSS image | |||
| ATCA | 2380 | 651.7 ± 19.6 | (Venturi et al. 2001) | ||||
| J 1324-3140 | A 3556 | GMRT | 235 | 77.1 ± 6.2 | 18.6 ± 1.5 | 58.5 ± 6.4 | This work |
| GMRT | 325 | 84.6 ± 4.2 | 16.8 ± 0.8 | 67.8 ± 4.3 | This work | ||
| GMRT | 610 | 18.7 ± 0.9 | 10.9 ± 0.5 | 7.8 ± 1.0 | This work | ||
| MOST | 843 | 16.7 ± 0.5 | SUMSS image | ||||
| ATCA | 1380 | 7.8 ± 0.2 | (Venturi et al. 1997) | ||||
| ATCA | 2380 | 7.4 ± 0.2 | (Venturi et al. 1997) | ||||
| ATCA | 4790 | 3.0 ± 0.1 | (Venturi et al. 2008) | ||||
| J 1327-3129b | A 3558 | GMRT | 235 | 19.1 ± 1.5 | This work | ||
| GMRT | 325 | 17.9 ± 1.4 | This work | ||||
| GMRT | 610 | 14.6 ± 0.7 | This work | ||||
| ATCA | 1380 | 6.2 ± 0.2 | (Venturi et al. 1997) | ||||
| ATCA | 2380 | 1.5 ± 0.1 | (Venturi et al. 1997) |
Notes. The flux density of the diffuse emission is the difference between the total flux density and the central emission, i.e. the emission contained within the optical counterpart, which is encompassed in the region highlighted in red in Figs. 6 and 7. The resolution of TGSS does not allow to separate J 1254-2900 and J 1254-2901a (A 3528 N). J 1254-2900 (A 3528 N) and J 1327-3129b (A 3558) do not show extended emission, and we provide only the total flux density. For J 1257-3021 (A 3532) we measured the flux density of the diffuse and central emission separately, and the total one as a sum of the two.
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