Table 4.
Integrated radio fluxes and radio power at 1.28 GHz.
Region | S410 | S650/700 | S1260 | S1284 | α | P1284 |
---|---|---|---|---|---|---|
[mJy] | [mJy] | [mJy] | [mJy] | [W Hz−1] | ||
A3528N | ||||||
J1254-2900 | 683.4 ± 54.9 | 408.6 ± 20.4 | 201.6 ± 10.1 | 277.4 ± 4.1 | −0.77 ± 0.07 | (1.6 ± 0.1)×1024 |
J1254-2901a | 299.1 ± 25.5 | 190.9 ± 9.6 | 100.1 ± 5.2 | 131.8 ± 8.0 | −0.70 ± 0.08 | (7.6 ± 0.4)×1023 |
J1254-2901b | 24.0 ± 5.4 | 18.2 ± 1.2 | 9.7 ± 1.0 | 15.8 ± 2.7 | −0.35 ± 0.22 | (9.0 ± 0.2)×1022 |
J1254-2904 | 742.4 ± 60.6 | 505.9 ± 25.4 | 264.5 ± 13.6 | 345.3 ± 18.4 | −0.66 ± 0.08 | (2.0 ± 0.1)×1024 |
A3528S | ||||||
J1254-2913 | 3949.6 ± 316.1 | 1892.3 ± 94.6 | 785.1 ± 39.3 | 1136.8 ± 60.0 | −1.09 ± 0.08 | (6.7 ± 0.3)×1024 |
mushroom NE | 366.1 ± 30.6 | 120.2 ± 6.5 | N/A | 38.8 ± 5.0 | −1.96 ± 0.13 | (2.4 ± 0.3)×1023 |
mushroom SE | 400.5 ± 33.2 | 110.0 ± 6.0 | N/A | 31.7 ± 4.7 | −2.23 ± 0.13 | (2.0 ± 0.3)×1023 |
filament N | 130.6 ± 17.4 | 33.0 ± 4.0 | N/A | 9.0 ± 7.2 | −2.34 ± 0.28 | (6.4 ± 0.4)×1022 |
filament S | 61.7 ± 9.8 | 21.1 ± 2.5 | N/A | 6.6 ± 4.3 | −1.93 ± 0.32 | (4.4 ± 2.4)×1022 |
J1254-2916 | 296.3 ± 27.3 | 148.9 ± 8.3 | 71.7 ± 3.6 | 103.2 ± 8.7 | −0.93 ± 0.11 | (6.0 ± 0.5)×1023 |
A3532 | ||||||
12547-3021 | 2934.7 ± 234.9 | 1795.2 ± 89.8 | 885.6 ± 44.3 | 1242.2 ± 62.3 | −0.75 ± 0.08 | (7.2 ± 0.4)×1023 |
filament N | 161.9 ± 14.6 | 36.8 ± 2.7 | N/A | 10.8 ± 4.6 | −2.38 ± 0.21 | (6.8 ± 2.8)×1022 |
filament S | 13.0 ± 0.1 | 2.6 ± 0.1 | N/A | 0.75 ± 0.05 | −2.49 ± 0.81 | (5.6 ± 2.1)×1021 |
Notes. Measurements were obtained from the regions drawn in the bottom panels in Fig. 5, at a common resolution of 12″. The radio powers were calculated using the integrated spectral index (α) obtained by fitting the radio flux densities with a power law in logarithm space (log S = β + α log ν) and listed in Column 6. For the uGMRT Band 5 at 1260 MHz, we measured the flux densities only for the radio galaxies (i.e. BCGs, HTs, NATs, and WATs) at full resolution (i.e. Θ1260 = 2.9″ × 2.2″).
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