Table B.1.
Candidate restarted radio galaxies.
| Name | Score, 1400 MHz | Score, 150 MHz | Stot, 1400 MHz | L150 MHz | M⋆ | Size |
|---|---|---|---|---|---|---|
| [mJy] | [mJy] | [mJy] | [×1025 WHz−1] | [×1011 M⊙] | [kpc] | |
| J102955+584621 | 0.42* | 4.33* | 4.8 | 1.5 ± 0.4 | – | 394 ± 31 |
| J103416+590523 | 0.61 | 3.43 | 3.3 | 1.3 ± 0.3 | 13 ± 13 | 490 ± 40 |
| J103508+583940 | 0.95 | 4.86 | 1.21 | 1.5 ± 0.2 | 4 ± 1 | 401.80 ± 0.06 |
| J103621+564323 | 0.70* | 62.11* | 58.3 | 33 ± 6 | 10 ± 4 | 1030 ± 40 |
| J103730+600011 | 0.87 | 3.40 | 2.9 | 0.0022 ± 0.0003 | 0.14 ± 0.02 | 35.40 ± 0.02 |
| J103815+601111 | 0.40* | 3.17 | 2.25* | 0.18 ± 0.02 | 1.0 ± 0.2 | 423.89 ± 0.08 |
| J103841+563544 | 1.26 | 1.49* | 1.8 | 2.7 ± 0.7 | 6 ± 7 | 670 ± 40 |
| J103845+594414 | 1.52 | 12.97 | 3.1 | 1.2 ± 0.2 | 1.9 ± 0.8 | 383 ± 18 |
| J104113+580755 | 2.42 | 5.63 | 4.3 | 1.3 ± 0.1 | 2.1 ± 0.5 | 1022.8 ± 0.1 |
| J104204+573449 | 1.28 | 6.29 | 4.9 | 1.6 ± 0.2 | 4 ± 2 | 514.07 ± 0.06 |
| J104252+553536 | 0.28* | 7.35* | 7.4 | 2.6 ± 0.3 | 12 ± 4 | 824.2 ± 0.2 |
| J104424+602917 | 1.08 | 4.16 | 6.3 | 0.7 ± 0.2 | 1.0 ± 0.3 | 378 ± 29 |
| J104520+563149 | 0.59 | 1.27 | 2.4 | 0.002 ± 0.014 | 0.05 ± 0.30 | 110 ± 340 |
| J104809+573010 | 0.34* | 1.18 | 2.25* | 0.80 ± 0.09 | 2.1 ± 0.5 | 828.0 ± 0.1 |
| J104834+560005 | 0.72 | 3.25 | 2.5 | 1.8 ± 0.3 | 26 ± 13 | 450 ± 8 |
| J104912+575014 | 1.57 | 9.66 | 2.6 | 0.15 ± 0.02 | 2.9 ± 0.5 | 147.24 ± 0.04 |
| J105057+562349 | 0.22* | 1.51 | 1.16* | 0.5 ± 0.1 | 8 ± 8 | 441 ± 22 |
| J105340+560950 | 1.27 | 7.73 | 3.0 | > 1.13 | > 11.9 | > 697 |
| J105418+595220 | 0.29* | 1.94 | 2.25* | 2.7 ± 0.4 | 3 ± 1 | 972 ± 17 |
| J105436+590901 | 4.38 | 4.64 | 5.2 | 2.5 ± 0.3 | – | 1046.9 ± 0.1 |
| J105524+561616 | 1.14 | 4.42 | 3.9 | 0.5 ± 0.1 | 3 ± 1 | 419 ± 26 |
| J105723+565938 | 0.77 | 10.93 | 1.38* | > 6.26 | > 16.6 | > 769 |
| J110021+601630 | 3.37* | 41.14* | 60.8 | 2.5 ± 0.3 | 1.1 ± 0.2 | 608.03 ± 0.07 |
Notes. The columns show: source name of the candidate restarted radio source; the core flux density measured directly in the FIRST image; the core flux density measured directly in the LOFAR 6″ image; total flux density value from the NVSS catalogue or image (see Sect. 4.3.1); radio luminosity of the source, stellar mass and the linear size of the radio galaxy. The asterisk denotes the upper limit values.
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