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Table 1.

Polarized GRGs.

GRG RA Dec z Ang. size Lin. size FR Remark
(deg) (deg) (arcsec) (Mpc)
1 164.273 53.440 0.460 (a) 153 0.92 II d
2 164.289 48.678 0.276 (a) 439 1.9 II d
7 164.575 51.672 0.415 (a) 330 1.86 II s
19 167.402 53.230 0.288 (b) 230 1.03 II d
22 168.381 46.371 0.589 (b) 112 0.76 II d
44 174.882 47.357 0.518 (a) 312 2.0 II s
47 178.000 49.849 0.891 (a) 96 0.77 II s
51 180.345 49.427 0.205 (b) 345 1.2 I d
57 182.692 53.490 0.448 (a) 119 0.71 I s
64 184.576 53.456 0.568 (c) 183 1.23 II d
65 184.708 50.438 0.199 (a) 210 0.71 II d
77 186.493 53.161 0.811 (c) 147 1.14 II d
80 187.498 53.546 0.523 (c) 137 0.88 II s
83 188.210 49.107 0.690 (a) 256 1.87 II s
85 188.756 53.299 0.345 (d) 683 3.44 II d
87 189.202 46.068 0.615 (b) 125 0.87 II d
91 190.052 53.577 0.293 (a) 164 0.74 II d
103 195.396 54.136 0.313 (b) 168 0.79 II d
112 197.620 52.228 0.650 (b) 197 1.41 II s
117 199.144 49.544 0.563 (b) 126 0.84 II core
120 200.124 49.280 0.684 (a) 113 0.82 II d
122 200.902 47.497 0.440 (b) 180 1.05 II s
136 203.345 53.547 0.354 (b) 173 0.88 s
137 203.549 55.024 1.245 (a) 91 0.78 II s
144 204.845 50.963 0.316 (b) 174 0.83 II d
145 205.263 49.267 0.747 (c) 113 0.85 II d
148 206.065 48.764 0.725 (b) 202 1.51 II s
149 206.174 50.383 0.763 (a) 123 0.93 II s
165 210.731 51.458 0.518 (c) 135 0.87 II d
166 210.813 51.746 0.485 (c) 228 1.41 II d
168 211.421 54.182 0.761 (c) 116 0.88 II d
177 213.535 48.699 1.361 (b) 107 0.92 II d
207 220.033 55.452 0.584 (c) 238 1.62 II s
222 222.739 53.002 0.918 (a) 184 1.48 II d
233 226.190 50.502 0.652 (c) 201 1.44 II d
234 226.553 51.619 0.611 (a) 262 1.82 II s
0 ( * ) 151.507 34.903 0.1005 (e) 2491 4.76 II d

Notes. Column 1: progressive GRG identification number from Table 2 in Dabhade et al. (2020); Cols. 2 and 3: J2000 celestial coordinates of the host galaxy. The reference is Dabhade et al. (2020) for all of the GRGs, apart from GRG 0 for which we refer to Becker et al. (1995); Col. 4: redshift (z); Cols. 5 and 6: angular and projected linear size; Col. 7: Fanaroff-Riley type (Fanaroff & Riley 1974). GRG 136 has a peculiar morphology and thus it is not classified; Col. 8: the letter indicates if the GRG is detected as a double (“d”) or a single (“s”) source in polarization. Polarized emission was detected from the core and/or inner jets region only in the case of GRG 117.

(a)

Spectroscopic redshifts from the Sloan Digital Sky Survey SDSS (York et al. 2000).

(b)

Redshifts from the LoTSS DR1 value-added catalog (Williams et al. 2019; Duncan et al. 2019).

(c)

Photometric redshifts from the SDSS.

(d)

Spectroscopic redshift from O’Sullivan et al. (2019).

(e)

Spectroscopic redshift from Hill et al. (1996).

( * )GRG 0 is 3C 236 that was added to the Dabhade et al. (2020) catalog for this analysis.

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