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Home All issues Volume 684 (April 2024) A&A, 684 (2024) A159 Full HTML
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Table 1.

3C sources considered ordered for increasing redshift.

3CR z FR Class Av SDSS NRS 3CR z FR Class Av SDSS NRS
129 0.0208 1 – 3.591 10±8 135 0.1253 2 HEG 0.373 27 ± 11
066B 0.0215 1 LEG 0.304 6 ± 20 424 0.127 2 LEG 0.319 75 ± 21
264 0.0217 1 – 0.078 17 ± 5 197.1 0.1301 2 BLO 0.139 ✓ 31 ± 13
129.1 0.0222 1 – 3.789 12 ± 7 223 0.1368 2 HEG 0.038 ✓ 35 ± 9
075N 0.0232 1 LEG 0.6 45 ± 8 089 0.1386 1 – 0.415 ✓ 94 ± 15
402 0.0239 1 – 0.399 22 ± 11 303 0.141 2 BLO 0.063 ✓ 45 ± 14
296 0.0240 1 LEG 0.084 0 ± 21 332 0.1517 2 BLO 0.077 ✓ 131 ± 17
083.1 0.0255 1 – 0.534 26 ± 10 348 0.154 1 ELEG 0.314 113 ± 19
442 0.0263 – LEG 0.213 24 ± 9 273 0.1583 – BLO 0.069 ✓ 38 ± 8
078 0.0286 1 LEG 0.565 10 ± 10 381 0.1605 2 HEG 0.174 116 ± 32
088 0.0302 2 LEG 0.417 −4 ± 4 346 0.161 2 – 0.224 ✓ 57 ± 14
338 0.0303 1 LEG 0.037 79 ± 10 357 0.1662 2 LEG 0.153 ✓ 123 ± 34
465 0.0303 1 LEG 0.234 87 ± 14 020 0.174 2 HEG 1.323 45 ± 15
353 0.0304 2 LEG 1.475 39 ± 12 219 0.1744 2 BLO 0.061 ✓ 49 ± 9
098 0.0304 2 HEG 0.741 −4 ± 6 063 0.175 2 HEG 0.086 30 ± 16
076.1 0.0324 1 – 0.451 7 ± 8 033.1 0.1809 2 BLO 2.007 32 ± 16
317 0.0345 – LEG 0.123 50 ± 14 061.1 0.184 2 HEG 0.570 18 ± 11
305 0.0416 2 HEG 0.08 10 ± 5 234 0.1848 2 HEG 0.062 ✓ 61 ± 10
029 0.0448 1 LEG 0.117 19 ± 13 018 0.188 2 BLO 0.535 7 ± 5
293 0.0450 – LEG 0.055 4 ± 10 319 0.192 2 – 0.041 ✓ 45 ± 10
318.1 0.0453 – – 0.118 49 ± 11 213.1 0.194 2 LEG 0.099 ✓ 43 ± 13
111 0.0485 2 BLO 5.458 21 ± 5 028 0.1952 2 ELEG 0.193 ✓ 87 ± 18
371 0.0500 – LEG 0.112 (127 ± 32) 34 ± 14 196.1 0.198 2 LEG 0.216 28 ± 9
310 0.0535 2 LEG 0.135 ✓ (70 ± 15) 25 ± 12 401 0.2010 2 LEG 0.193 48 ± 19
430 0.0541 2 LEG 2.035 (353 ± 146) 40 ± 7 349 0.205 2 LEG 0.105 ✓ 46 ± 11
403.1 0.055 2 LEG 0.760 (448 ± 99) 18 ± 9 132 0.214 2 LEG 1.632 39 ± 33
390.3 0.0561 2 BLO 0.236 (240 ± 39) 66 ± 11 436 0.2145 2 HEG 0.298 ✓ 20 ± 9
445 0.0562 2 BLO 0.275 (47 ± 14) 12 ± 11 287.1 0.2159 2 BLO 0.082 ✓ 47 ± 11
382 0.0578 2 BLO 0.231 (50 ± 29) 0 ± 7 123 0.2177 – LEG 3.233 19 ± 8
403 0.0590 2 HEG 0.626 (368 ± 181) 6 ± 6 017 0.2198 2 BLO 0.077 ✓ 38 ± 9
033 0.0596 2 HEG 0.071 (72 ± 13) 34 ± 9 459 0.2199 2 BLO 0.216 19 ± 7
192 0.0598 2 HEG 0.183 ✓ (22 ± 14) −2 ± 4 180 0.2200 2 HEG 0.325 12 ± 12
136.1 0.064 2 HEG 2.494 (135 ± 34) 9 ± 3 456 0.2330 2 HEG 0.123 8 ± 7
035 0.0670 2 – 0.461 (122 ± 50) 15 ± 5 171 0.2384 HEG 9 ± 7
015 0.073 1 LEG 0.071 ✓ (29 ± 14) 10 ± 9 284 0.2394 2 HEG 0.052 ✓ 24 ± 8
285 0.0794 2 HEG 0.056 ✓ (40 ± 15) 24 ± 7 093.1 0.2430 – HEG 1.283 27 ± 9
452 0.0811 2 HEG 0.459 (84 ± 30) 33 ± 10 166 0.2449 2 LEG 0.673 23 ± 12
198 0.0815 2 SF 0.086 ✓ (72 ± 20) 37 ± 7 288 0.246 1 LEG 0.026 ✓ 22 ± 12
277.3 0.0857 2 HEG 0.038 ✓ (46 ± 24) 24 ± 14 410 0.249 2 BLO 4.521 25 ± 10
227 0.0861 2 BLO 0.085 ✓ (46 ± 10) 38 ± 7 079 0.2559 2 HEG 0.424 7 ± 6
105 0.089 2 HEG 1.588 (34 ± 11) 25 ± 6 379.1 0.256 2 HEG 0.201 18 ± 10
326 0.0895 2 LEG 0.170 ✓ (54 ± 13) 40 ± 9 323.1 0.264 – BLO 0.141 ✓ 21 ± 7
388 0.091 2 LEG 0.260 (171 ± 25) 80 ± 10 303.1 0.267 2 HEG 0.120 10 ± 6
321 0.096 2 LEG 0.145 ✓ (27 ± 9) 13 ± 5 460 0.268 2 LEG 0.297 12 ± 6
236 0.1005 2 LEG 0.036 ✓ 25 ± 10 300 0.27 2 HEG 0.116 ✓ 27 ± 11
433 0.1016 1–2 HEG 0.483 109 ± 37 153 0.2769 2 LEG 0.537 50 ± 12
327 0.1041 2 HEG 0.295 74 ± 16 133 0.2775 2 HEG 2.967 21 ± 9
223.1 0.107 2 HEG 0.058 ✓ 30 ± 10 052 0.2854 2 – 0.789 28 ± 10
315 0.1083 – LEG 0.205 ✓ 67 ± 16 458 0.289 2 HEG 0.277 12 ± 9
130 0.1090 1 – 4.535 56 ± 17 438 0.290 1 – 1.221 109 ± 20
184.1 0.1182 2 BLO 0.108 23 ± 10 173.1 0.2921 LEG 8 ± 9
314.1 0.1197 – ELEG 0.063 45 ± 9 165 0.2957 2 LEG 0.572 21 ± 12

Notes. The number of sources in the RS (NRS) for RGs at z > 0.05 is the one found with the first method, without selecting just the extended sources. Column description: (1) Source name; (2) Redshift; (3) FR classification; (4) Optical spectroscopic classification; (5) Galactic absorption in magnitudes; (6) Availability of SDSS data; (7) Number of RS sources subtracted to the ground. Values outside the parenthesis refer to the estimates of NRS obtained by selecting only extended optical sources for the sources with 0.05 < z < 0.1.

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