Table 7
Polarized sources in the ELAIS-N1 LOFAR Deep Field that might be located behind or are embedded within the galaxy clusters identified by Zou et al. 2022 (Clustering by Fast Search and Find of Density Peaks; CFSFDP) and/or Wen & Han 2024 (WH).
| Source | Source redshift | Cluster | Cluster redshift | R200(a) | θsep(b) | dsep(c) |
|---|---|---|---|---|---|---|
| (Mpc) | (arcsec) | (Mpc) | ||||
| 07 | 0.7683 | CFSFDP 464000084 | 0.2440 | 1.14 | 196 | 0.75 |
| 10 | 1.9482 | WHJ160827.0+561505 | 0.5396 | 0.78 | 85 | 0.54 |
| 16* | 0.32936 | WHJ161531.1+545230 | 0.3294 | 0.72 | 10 | 0.05 |
| 18* | 0.24297 | WHJ161623.7+552702 | 0.2430 | 0.85 | 0 | 0 |
| 19 | 0.7523 | WH J161832.0+543337 | 0.3918 | 0.88 | 94 | 0.50 |
| WH J161820.9+543040 | 0.7944 | 1.09 | 136 | 1.02 | ||
| 22 | 0.4910 | CFSFDP 483700074 | 0.4672 | 0.84 | 27 | 0.16 |
| 26* | 0.3566 | WH J160929.8+552542 | 0.2602 | 0.87 | 108 | 0.43 |
| WH J160919.5+552549 | 0.3572 | 0.74 | 169 | 0.85 | ||
| 28 | 0.48882 | CFSFDP 445000147 | 0.2234 | 1.40 | 146 | 0.52 |
| 32* | 0.21431 | WH J161858.7+545228 | 0.2139 | 0.86 | 1 | 0.003 |
Notes. Sources with an asterisk are in a cluster. Three of these (sources 16, 18, and 32) are associated with radio galaxies whose host galaxy is the brightest cluster galaxy. (a)R200 = R500/0.7, calculated from the R500 values given by the authors in their adopted cosmology (footnote 8).(b) Angular separation between the polarized source and the cluster center. (c)Projected linear separation between the polarized source and the cluster center.
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