Table C.1.
Sample of radio halos and candidate radio halos that were classified with an asterisk (the RH* and cRH* in Table A.1) because of their low significance. The integrated flux density of these sources cannot be determined accurately with current data.
| Name | S150 (2σ) | S150err (2σ) | S150 (fit) | S150err (fit) | P150 | P150err | I0 | I0err | r1 | r1err | Model | S/N | rms |  |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| [mJy] | [mJy] | [mJy] | [mJy] | [W Hz−1] | [W Hz−1] | [μJy arcsec−2] | [μJy arcsec−2] | [kpc] | [kpc] | [mJy beam−1] | ||||
| PSZ2 G071.39+59.54 | 20.01 | 2.30 | 88.87 | 11.90 | 2.60e+25 | 3.48e+24 | 1.27 | 0.08 | 529.2 | 36.0 | circle | 11.25 | 0.319 | 1.15 |
| PSZ2 G076.55+60.29 | 8.14 | 1.67 | 22.52 | 5.72 | 6.33e+24 | 1.61e+24 | 0.43 | 0.07 | 453.8 | 82.3 | circle | 4.40 | 0.118 | 0.76 |
| PSZ2 G077.90-26.63 | 28.02 | 4.04 | 64.10 | 10.75 | 3.89e+24 | 6.52e+23 | 1.88 | 0.24 | 218.1 | 26.5 | circle | 7.53 | 0.439 | 1.03 |
| PSZ2 G095.29+44.13 | 13.82 | 2.08 | 27.38 | 4.36 | 1.08e+25 | 1.72e+24 | 1.21 | 0.13 | 328.7 | 32.8 | circle | 8.48 | 0.266 | 0.89 |
| PSZ2 G099.55+34.23 | 13.48 | 5.97 | 93.17 | 19.09 | 3.14e+25 | 6.44e+24 | 0.56 | 0.07 | 851.0 | 112.6 | circle | 5.95 | 0.237 | 0.84 |
| PSZ2 G116.50-44.47 | 12.62 | 6.73 | 23.23 | 8.29 | 1.42e+25 | 5.05e+24 | 3.94 | 0.78 | 187.8 | 36.0 | circle | 5.11 | 0.680 | 1.08 |
| PSZ2 G118.34+68.79 | 7.31 | 2.48 | 25.05 | 4.47 | 5.33e+24 | 9.52e+23 | 0.80 | 0.09 | 321.5 | 32.4 | circle | 8.58 | 0.208 | 1.34 |
| PSZ2 G123.00-35.52 | 8.28 | 1.86 | 20.43 | 4.27 | 1.13e+25 | 2.35e+24 | 2.23 | 0.35 | 228.4 | 34.4 | circle | 5.93 | 0.578 | 1.08 |
| PSZ2 G133.59+50.68 | 10.19 | 1.45 | 18.96 | 3.35 | 2.37e+25 | 4.18e+24 | 1.20 | 0.15 | 362.8 | 43.6 | circle | 7.07 | 0.257 | 0.92 |
| PSZ2 G163.61+34.30 | 8.50 | 2.19 | 17.02 | 3.71 | 2.87e+25 | 6.25e+24 | 1.50 | 0.24 | 324.7 | 44.9 | circle | 6.21 | 0.379 | 0.79 |
Notes. Col. 1: PSZ2 name; Cols. 2 and 3: flux density integrated within the 2σ region and its error; Cols. 4 and 5: flux density obtained from the surface brightness profile fitting and its error; Cols. 6 and 7: radio power and its error; Cols. 8 and 9: best-fit central brightness and its error; Cols. 10 and 11: best-fit e-folding radius and its error; Col. 12: model adopted for the fitting; Col. 13: S/N of the radio halo; Col. 14: rms noise of the image used to fit the surface brightness profile; Col. 15: 
of the fit.
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