Open Access
Table C.2.
Best-fit values of the elliptical exponential model for each radio halo considered.
| Name | PRH (1024 W Hz−1) | I0 (μJy arcsec−2) | r1 (kpc) | r2 (kpc) | S/N | χ2 |
|---|---|---|---|---|---|---|
| PSZ2G008.31-64.74 | 7.06 ± 0.48 | 0.23 ± 0.01 | 1003 ± 59 | 376 ± 25 | 30.4 | 0.96 |
| PSZ2G008.94-81.22 | 16.35 ± 1.06 | 2.80 ± 0.09 | 293 ± 12 | 246 ± 10 | 41.8 | 0.54 |
| PSZ2G056.93-55.08 | 10.24 ± 0.65 | 0.83 ± 0.02 | 364 ± 23 | 270 ± 21 | 51.0 | 1.53 |
| PSZ2G159.91-73.50 | 1.96 ± 0.35 | 0.55 ± 0.30 | 306 ± 115 | 205 ± 58 | 6.0 | 2.09 |
| PSZ2G172.98-53.55 | 2.63 ± 0.21 | 0.46 ± 0.04 | 278 ± 46 | 204 ± 44 | 19.0 | 0.59 |
| PSZ2G205.93-39.46 | 11.02 ± 0.95 | 1.67 ± 0.15 | 310 ± 29 | 172 ± 19 | 16.1 | 0.53 |
| PSZ2G208.80-30.67 | 1.97 ± 0.68 | 0.38 ± 1.45 | 349 ± 249 | 226 ± 145 | 3.0 | 2.13 |
| PSZ2G225.93-19.99 | 12.98 ± 0.78 | 2.30 ± 0.02 | 264 ± 10 | 177 ± 10 | 148.2 | 3.07 |
| PSZ2G239.27-26.01 | 7.83 ± 0.48 | 1.33 ± 0.02 | 273 ± 11 | 181 ± 10 | 108.0 | 1.32 |
| PSZ2G243.15-73.84 | 3.87 ± 0.25 | 0.57 ± 0.02 | 315 ± 20 | 193 ± 11 | 41.1 | 3.81 |
| PSZ2G259.98-63.43 | 9.49 ± 0.65 | 6.12 ± 0.30 | 158 ± 9 | 131 ± 9 | 30.9 | 0.59 |
| PSZ2G262.27-35.38 | 5.28 ± 0.35 | 0.27 ± 0.01 | 731 ± 37 | 340 ± 22 | 37.1 | 1.01 |
| PSZ2G263.68-22.55 | 9.66 ± 0.72 | 1.30 ± 0.07 | 598 ± 43 | 251 ± 14 | 22.5 | 0.70 |
| PSZ2G266.04-21.25 | 25.46 ± 1.60 | 5.72 ± 0.15 | 304 ± 11 | 187 ± 8 | 52.0 | 0.84 |
| PSZ2G277.76-51.74 | 6.25 ± 0.44 | 0.28 ± 0.02 | 440 ± 31 | 409 ± 33 | 27.2 | 0.94 |
| PSZ2G278.58+39.16 | 13.55 ± 0.82 | 4.74 ± 0.04 | 200 ± 10 | 177 ± 10 | 183.0 | 2.80 |
| PSZ2G286.98+32.90 | 28.35 ± 1.71 | 2.36 ± 0.02 | 389 ± 7 | 293 ± 7 | 177.8 | 1.57 |
| PSZ2G313.33+61.13 | 2.21 ± 0.13 | 1.40 ± 0.02 | 204 ± 10 | 146 ± 10 | 102.3 | 0.83 |
| PSZ2G313.88-17.11 | 2.95 ± 0.28 | 1.54 ± 0.12 | 265 ± 31 | 153 ± 16 | 13.8 | 0.28 |
| PSZ2G346.61+35.06 | 3.37 ± 0.21 | 0.34 ± 0.01 | 419 ± 12 | 393 ± 13 | 61.0 | 0.90 |
| PSZ2G349.46-59.95 | 3.81 ± 0.27 | 1.44 ± 0.08 | 190 ± 12 | 151 ± 11 | 27.0 | 0.48 |
References. (1) cluster name; (2) total radio halo power at 1.28 GHz; (3) radio halo central surface brightness; (4-5) e-folding radii; (6) signal-to-noise ratio of the emission; (7) reduced chi-square of the fit.
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