Table C.1.
First 30 rows of the catalogue of 819 polarised radio sources that were detected in this work.
| RA [deg] | DEC [deg] | Maj [″] | Min [″] | PA [deg] | p0 | χ0 [rad] | RM [rad m−2] | σRM [rad m−2] | I0 [mJy] | α |  |
zbest | zbest source | θp [arcmin] | r/R500 | Cluster | RAopt [deg] | DECopt [deg] | Multi component | Flagged | Note |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| -132.2610 | 5.6140 | 8.2 | 5.8 | 90 |
 |
 |
 |
 |
 |
 |
171 | 0.584 ± 0.040 | 2 | 8.06 | 0.6 | G006.47+50.54 | 227.7304 | 5.6153 | True | True | |
| -132.2780 | 5.6184 | 4.9 | 4.0 | 52 |
 |
 |
 |
 |
 |
 |
56 | 0.584 ± 0.040 | 2 | 7.80 | 0.6 | G006.47+50.54 | 227.7304 | 5.6153 | True | False | |
| -132.2767 | 5.6172 | 5.4 | 3.8 | 68 |
 |
 |
 |
 |
 |
 |
66 | 0.584 ± 0.040 | 2 | 7.87 | 0.6 | G006.47+50.54 | 227.7304 | 5.6153 | True | False | |
| -111.9212 | 5.5698 | 6.2 | 5.7 | 59 |
 |
 |
 |
 |
 |
 |
75 | 0.581 ± 1.268 | 2 | 6.10 | 0.8 | G021.09+33.25 | 248.0775 | 5.5694 | False | False | Counterpart unsure |
| -111.9898 | 5.4658 | 7.8 | 5.9 | 41 |
 |
 |
 |
 |
 |
 |
104 | 1.675 ± 0.611 | 2 | 12.44 | 1.7 | G021.09+33.25 | 248.0106 | 5.4644 | True | True | |
| -111.7294 | 5.5442 | 12.0 | 6.5 | 76 |
 |
 |
 |
 |
 |
 |
151 | - | - | 6.00 | 0.8 | G021.09+33.25 | - | - | False | True | No optical counterpart. |
| -111.9211 | 5.4755 | 7.1 | 6.3 | 39 |
 |
 |
 |
 |
 |
 |
131 | 2.389 ± 0.208 | 2 | 8.98 | 1.2 | G021.09+33.25 | - | - | False | True | No optical counterpart. |
| -111.9888 | 5.4639 | 7.7 | 6.2 | 49 |
 |
 |
 |
 |
 |
 |
152 | 1.675 ± 0.611 | 2 | 12.46 | 1.7 | G021.09+33.25 | 248.0106 | 5.4644 | True | True | |
| -48.0417 | -17.7068 | 7.7 | 7.1 | 111 |
 |
 |
 |
 |
 |
 |
57 | - | - | 8.50 | 1.4 | G028.77-33.56 | - | - | False | True | No optical counterpart. |
| -47.9835 | -17.7248 | 7.2 | 7.2 | 103 |
 |
 |
 |
 |
 |
 |
73 | - | - | 5.66 | 0.9 | G028.77-33.56 | - | - | False | False | No optical counterpart. |
| -48.0167 | -17.7220 | 7.8 | 6.5 | 89 |
 |
 |
 |
 |
 |
 |
59 | - | - | 6.87 | 1.1 | G028.77-33.56 | - | - | False | False | No optical counterpart. |
| -119.4219 | 16.0547 | 8.8 | 8.5 | 27 |
 |
 |
 |
 |
 |
 |
215 | 0.282 ± 0.077 | 2 | 0.95 | 0.0 | G029.00+44.56 | 240.5791 | 16.0553 | False | True | Counterpart unsure |
| -119.3140 | 16.1258 | 7.9 | 5.5 | 74 |
 |
 |
 |
 |
 |
 |
68 | - | - | 8.37 | 0.3 | G029.00+44.56 | - | - | False | True | No optical counterpart. |
| -119.6253 | 16.0712 | 8.4 | 8.0 | 94 |
 |
 |
 |
 |
 |
 |
235 | 1.285 ± 0.435 | 2 | 10.83 | 0.4 | G029.00+44.56 | - | - | False | True | No optical counterpart. |
| -119.4438 | 15.8343 | 7.9 | 6.2 | 40 |
 |
 |
 |
 |
 |
 |
61 | - | - | 13.16 | 0.5 | G029.00+44.56 | - | - | False | False | No optical counterpart. |
| -119.4234 | 16.1195 | 8.5 | 8.3 | 66 |
 |
 |
 |
 |
 |
 |
163 | 0.385 ± 0.000 | 0 | 4.05 | 0.2 | G029.00+44.56 | 240.5783 | 16.1194 | False | True | |
| -152.5871 | 26.5863 | 6.1 | 5.3 | 137 |
 |
 |
 |
 |
 |
 |
57 | - | - | 9.07 | 0.6 | G033.78+77.16 | - | - | False | False | No optical counterpart. |
| -152.7815 | 26.5929 | 18.0 | 9.2 | 176 |
 |
 |
 |
 |
 |
 |
733 | 0.250 ± 0.114 | 2 | 1.45 | 0.1 | G033.78+77.16 | 207.2186 | 26.5931 | False | True | |
| -152.6178 | 26.5824 | 6.1 | 6.0 | 176 |
 |
 |
 |
 |
 |
 |
107 | 0.793 ± 0.078 | 2 | 7.43 | 0.5 | G033.78+77.16 | 207.3823 | 26.5824 | False | False | |
| -152.5220 | 26.5313 | 7.0 | 6.1 | 82 |
 |
 |
 |
 |
 |
 |
80 | 1.187 ± 0.378 | 2 | 12.97 | 0.9 | G033.78+77.16 | - | - | False | False | No optical counterpart. |
| -152.8105 | 26.5899 | 5.4 | 5.0 | 68 |
 |
 |
 |
 |
 |
 |
71 | 0.570 ± 0.000 | 0 | 2.93 | 0.2 | G033.78+77.16 | 207.1893 | 26.5903 | False | False | |
| -152.5875 | 26.6306 | 7.5 | 6.9 | 62 |
 |
 |
 |
 |
 |
 |
160 | - | - | 9.46 | 0.6 | G033.78+77.16 | - | - | False | True | No optical counterpart. |
| -2.0992 | -25.9382 | 7.7 | 5.8 | 102 |
 |
 |
 |
 |
 |
 |
68 | 0.187 ± 0.133 | 3 | 8.47 | 2.0 | G034.03-76.59 | 357.9006 | -25.9388 | False | False | |
| -89.0409 | 10.0803 | 7.5 | 4.7 | 66 |
 |
 |
 |
 |
 |
 |
82 | 0.559 ± 0.089 | 3 | 10.82 | 1.7 | G036.72+14.92 | - | - | False | False | No optical counterpart. |
| -88.7551 | 10.1938 | 7.6 | 5.5 | 150 |
 |
 |
 |
 |
 |
 |
70 | 0.416 ± 0.214 | 3 | 11.41 | 1.8 | G036.72+14.92 | 271.2446 | 10.1943 | False | False | |
| -88.8378 | 9.9030 | 6.4 | 5.3 | 59 |
 |
 |
 |
 |
 |
 |
77 | 0.186 ± 0.073 | 3 | 8.13 | 1.3 | G036.72+14.92 | 271.1620 | 9.9031 | False | False | |
| -88.7312 | 9.9649 | 8.3 | 4.7 | 48 |
 |
 |
 |
 |
 |
 |
81 | - | - | 8.90 | 1.4 | G036.72+14.92 | 271.2703 | 9.9618 | True | False | |
| -88.7910 | 10.1261 | 13.6 | 7.3 | 57 |
 |
 |
 |
 |
 |
 |
108 | 0.130 ± 0.032 | 3 | 6.88 | 1.1 | G036.72+14.92 | 271.2022 | 10.1263 | True | False | |
| -88.7946 | 10.1282 | 13.6 | 6.4 | 67 |
 |
 |
 |
 |
 |
 |
99 | 0.130 ± 0.032 | 3 | 6.85 | 1.1 | G036.72+14.92 | 271.2022 | 10.1263 | True | False | |
| -88.8257 | 10.0041 | 14.9 | 8.0 | 172 |
 |
 |
 |
 |
 |
 |
10001 | - | - | 2.94 | 0.5 | G036.72+14.92 | 271.1741 | 10.0012 | True | True |
Notes. The full table is available in electronic form at the CDS. The columns ‘Maj’ and ‘Min’ indicate the major and minor axis of the polarised sources and ‘PA’ the position angle. The results of the fitting as described in Section 3.2 are given in the columns p0 to 
with uncertainties given by the 16th and 84th percentile of the MCMC chains. The columns starting with z are the results of the redshift estimates as detailed in Section 3.4. The angular distance to the pointing centre and projected radius to the cluster centre are given by the θp and r/R500 columns respectively. The ‘Flagged’ column indicates True when the source was omitted for the final analysis, for example because it was a bad fit.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.