Table A.1
Catalog of properties of polarized sources in the ELAIS-Nl LOFAR deep field.
Source | RM | GRM | RRM | Angular size | Linear size | Flux | log10(Luminosity) | Redshift | Redshift type | Host classification | Radio morphology |
---|---|---|---|---|---|---|---|---|---|---|---|
(rad m−2) | (rad m−2) | (rad m−2) | (arcsec) | (kpc) | (mJy) | ||||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
01 | 1.68 ±0.02 | 1.63 ± 2.01 | 0.05 ± 2.01 | 17 | 91 | 163 | 25.89 | 0.37779 | s | QSO | FRII |
02(*) | 9.71 ± 0.05 | 4.41 ± 2.78 | 5.30 ± 2.78 | 35 | 285 | 471 | 27.30 | 0.98 | P | QSO | FRII |
03 | −5.83 ± 0.02 | −3.91 ± 2.69 | −1.92 ±2.69 | 10 | 45 | 602 | 26.23 | 0.3 | s | Bl | OE |
04A | 19.68 ±0.01 | 14.47 ± 2.83 | 5.21 ± 2.83 | 77 | 349 | 1737 | 26.66 | 0.29186 | s | QSO | FRII |
04B | 21.78 ±0.01 | 14.47 ± 2.83 | 7.31 ± 2.83 | 77 | 349 | 1737 | 26.66 | 0.29186 | s | QSO | FRII |
05 | 19.12 ±0.05 | 9.91 ± 2.81 | 9.21 ± 2.81 | 33 | 233 | 196 | 26.49 | 0.6359 | s | G | FRII |
06 | 18.43 ±0.03 | 11.01 ± 2.84 | 7.42 ± 2.84 | 300 | 378 | 209 | 24.32 | 0.06333 | s | G | FRI |
07 | 6.062 ± 0.003 | 5.17 ± 2.15 | 0.89 ± 2.15 | 12 | 91 | 1299 | 27.51 | 0.7683 | s | G | FRII |
08 | 13.39 ±0.03 | 7.66 ± 2.26 | 5.73 ± 2.26 | 61 | 521 | 338 | 27.36 | 1.197 | s | G | FRII |
09 | −3.79 ± 0.03 | 2.10 ± 2.55 | −5.89 ± 2.55 | 1 | 9 | 24 | 25.82 | 0.81512 | s | G | C |
10 | −5.61 ±0.05 | 0.22 ± 2.43 | −5.83 ± 2.43 | 3 | 27 | 122 | 27.40 | 1.94822 | s | Bl | C |
11 | −6.24 ± 0.04 | 0.59 ± 2.45 | −6.83 ± 2.45 | 152 | 1308 | 511 | 27.63 | 1.32046 | s | QSO | FRII |
12 | 7.17 ±0.02 | 7.93 ± 2.23 | −0.76 ± 2.23 | 142 | 1169 | 458 | 27.30 | 0.99258 | s | QSO | FRII |
13A | 2.38 ± 0.04 | 5.70 ± 2.47 | −3.32 ± 2.47 | 129 | 956 | 41 | 25.92 | 0.71385 | s | QSO | FRII |
14 | 10.31 ±0.02 | 9.16 ± 2.93 | 1.15 ± 2.93 | 53 | 130 | 122 | 24.78 | 0.13455 | s | G | FRI |
15(*) | −4.80 ± 0.04 | 1.49 ± 1.99 | −6.29 ± 1.99 | 96 | 769 | 70 | 26.38 | 0.9 | P | G | FRII |
16 | −4.01 ± 0.05 | 5.17 ± 2.39 | −9.18 ± 2.39 | 45 | 220 | 74 | 25.41 | 0.32936 | s | G | OE |
17 | 1.95 ±0.03 | 2.42 ± 1.78 | −0.47 ± 1.78 | 64 | 315 | 118 | 25.63 | 0.3347 | s | G | FRII |
18 | −20.31 ± 0.03 | 3.78 ± 2.33 | −24.09 ± 2.33 | 144 | 569 | 167 | 25.48 | 0.24297 | s | G | FRI |
19 | 2.91 ± 0.04 | 6.46 ± 2.68 | −3.55 ± 2.68 | 30 | 227 | 260 | 26.78 | 0.7523 | s | G | FRII |
20 | −4.70 ± 0.02 | 4.52 ± 2.34 | −9.22 ± 2.34 | 36 | 313 | 144 | 27.34 | 1.6981 | s | Bl | OE |
21(*) | 3.29 ± 0.04 | 9.52 ±3.19 | −6.23 ±3.19 | 27 | 226 | 348 | 27.28 | 1.09 | P | G | FRII |
22 | 2.31 ± 0.05 | 9.79 ± 3.07 | −7.48 ± 3.07 | 15 | 93 | 93 | 25.90 | 0.491 | s | G | OE |
23 | 5.91 ±0.05 | 6.15 ± 2.63 | −0.24 ± 2.63 | 257 | 2089 | 67 | 26.41 | 0.9443 | s | G | FRII |
24 | 9.43 ± 0.01 | 8.02 ±2.17 | 1.41 ± 2.17 | 6 | 34 | 258 | 26.18 | 0.415 | P | Bl | C |
25 | 10.03 ± 0.02 | 7.46 ± 2.87 | 2.57 ± 2.87 | 6 | 53 | 135 | 26.91 | 1.1326 | s | QSO | C |
26 | −5.38 ± 0.07 | 2.72 ± 2.60 | −8.10 ± 2.61 | 158 | 817 | 215 | 25.95 | 0.3566 | s | QSO | FRII |
27 | 14.17 ±0.07 | 9.84 ± 2.92 | 4.33 ± 2.92 | 111 | 141 | 190 | 24.30 | 0.06389 | s | G | FRII |
28 | −5.74 ± 0.05 | 2.40 ± 2.57 | −8.14 ±2.57 | 8 | 51 | 68 | 25.76 | 0.48882 | s | G | OE |
29 (13B) | 3.92 ± 0.05 | 5.70 ± 2.47 | −1.78 ± 2.47 | 129 | 956 | 41 | 25.92 | 0.71385 | s | QSO | FRII |
30(*) | 19.40 ± 0.07 | 11.82 ±3.45 | 7.58 ± 3.45 | 30 | 235 | 207 | 26.78 | 0.83 | P | G | FRII |
31 | 6.23 ± 0.06 | 8.75 ± 2.89 | −2.52 ± 2.89 | 38 | 315 | 328 | 27.23 | 1.0524 | s | G | FRII |
32 | −4.05 ± 0.06 | 5.74 ± 2.48 | −9.79 ± 2.48 | 140 | 504 | 116 | 25.20 | 0.21431 | s | G | FRI |
(1) Name of polarized source, as in Paper I; Source 04A and 04B are two lobes of the same radio galaxy; Source 13A and 29 (or 13B) are two lobes of the same radio galaxy; (2) RM and RM error of polarized source, from Paper I; (3) GRM and GRM error at the location of the polarized sources; (4) RRM and RRM error at the location of the polarized sources; (5) angular size of radio galaxy, including components undetected in polarization; (6) projected linear size of radio galaxy, including components undetected in polarization; (7) flux density in Stokes / integrated over the radio source; (8) logarithm of rest-frame luminosity in W Hz−1 at 146 MHz; (9) redshift of host galaxy; (10) redshift type, p = photometric redshift, s = spectroscopic redshift; (11) Host classification, QSO = Quasi-Stellar Object, Bl = blazar, G = galaxy; (12) Radio morphology classification at 146 MHz, C = compact, OE = other extended, FRI = FRI radio galaxy, FRII = FRII radio galaxy.
(*) The photometric redshifts of these sources are from Simonte et al. (2024), who determined them by averaging the photometric redshifts from multiple catalogs. The full Table and references are available at the CDS.
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