Table 2.
Properties and (tentative) classification of the analysed radio sources.
| Host | Reg. | Class. | Dc | LLS | A | S144 | S400 | α | P150 |
|---|---|---|---|---|---|---|---|---|---|
| (kpc) | (kpc) | (103 kpc2) | (mJy) | (mJy) | (1024 W Hz−1) | ||||
| G071 | - | RP(c,∗) | 920+ | 580 | 78 | 197.8 ± 19.8 | 19.5 ± 1.2 | 2.3 ± 0.1 | 14.6 ± 1.5 |
| G088 | A, B | HT(∗) | 290+ | 275 | 29 | 431.1 ± 43.1 | 74.7 ± 4.5 | 1.7 ± 0.1 | 20.6 ± 2.1 |
| G088 | C, D | GReET(c,∗) | 155+ | 315 | 28 | 123.1 ± 12.3 | 6.1 ± 0.4 | 2.9 ± 0.1 | 6.5 ± 0.6 |
| G088 | E | Uncertain | 390+ | 215 | 21 | 432.1 ± 43.2 | 121.6 ± 7.3 | 1.2 ± 0.1 | 19.8 ± 2.0 |
| G088 | S2 | Uncertain | 535+ | 210 | 14 | 24.6 ± 2.5 | 2.4 ± 0.2 | 2.3 ± 0.1 | 1.3 ± 0.2 |
| G113 | – | Remnant | 580+ | 210 | 21 | 48.4 ± 5.0 | 13.1 ± 0.8 | 1.3 ± 0.1 | 1.4 ± 0.1 |
| G137 | A | Uncertain(∗) | 240+ | 130 | 6 | 342.0 ± 34.2 | 86.0 ± 5.2 | 1.4 ± 0.1 | 6.3 ± 0.6 |
| G137 | B, Fil. | WAT(∗) | 300+ | 280 | 17 | 403.7 ± 40.4 | 99.7 ± 6.0 | 1.4 ± 0.1 | 7.4 ± 0.7 |
| G155 | A | HT | 435x | 285 | 41 | 581.5 ± 58.2 | 254.0 ± 15.2 | 0.8 ± 0.1 | 195.2 ± 20.3 |
| G155 | B | Remnant | 520x | 430 | 53 | 85.8 ± 8.6 | 5.6 ± 0.4 | 2.7 ± 0.1 | 46.0 ± 4.8 |
| G165 | A | Remnant | 750x | 240 | 23 | 56.7 ± 5.7 | 12.1 ± 0.7 | 1.5 ± 0.1 | 7.6 ± 0.8 |
| G165 | B | Remnant | 720x | 260 | 25 | 61.6 ± 6.2 | 9.5 ± 0.6 | 1.8 ± 0.1 | 8.6 ± 0.8 |
| G172 | A | NAT | 40+ | 90 | 7 | 4104.4 ± 410.4 | 2020.9 ± 121.3 | 0.7 ± 0.1 | 60.0 ± 6.0 |
| G172 | B, C, D | Uncertain | 40+ | 220 | 21 | 2116.1 ± 211.6 | 460.1 ± 27.6 | 1.5 ± 0.1 | 32.8 ± 3.2 |
Notes. Cols. 1–2: Host cluster and considered region of the radio source. Col. 3: (Tentative) classification; c stands for candidate, and the asterisk indicates evidence of re-energising based on radio data alone (not considering X-rays). Cols. 4–6: Projected distance of the target from the Planck centre (x) or X-ray peak (+), largest linear size, and area. Cols. 7–10: Flux densities measured within regions encompassing the 3σ level of the 144 MHz image, integrated spectral index, and k-corrected radio power at 150 MHz.
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