Table 2.
Candidate restarted radio galaxies selected with the different criteria described in Sect. 4.3.
Name | redshift | Sint, 150 MHz | CP1400 MHz | SB150 MHz | αinner region | Selection |
---|---|---|---|---|---|---|
[mJy] | [mJy arcmin−2] | criteria | ||||
J103416+590523 | 0.47 ± 0.06p | 29.54 | 0.19 | 47 | – | CP |
J103508+583940 | 0.4709 ± 0.0001s | 34.17 | 0.80 | 46 | – | CP |
J103730+600011 | 0.02815 ± 0.00002s | 12.57 | 0.30 | 38 | – | CP |
J103841+563544 | 0.57 ± 0.07p | 44.04 | 0.70 | 50 | – | CP |
J104113+580755 | 0.30894 ± 0.00006s | 64.17 | 0.56 | 21 | – | CP |
J104204+573449 | 0.4808 ± 0.0001s | 34.81 | 0.26 | 21 | – | CP |
J104424+602917 | 0.22 ± 0.02p | 68.18 | 0.17 | 40 | – | CP |
J104520+563149 | 0.034 ± 0.1p | 35.42 | 0.20 | 22 | – | CP |
J104834+560005 | 0.796 ± 0.04p | 16.48 | 0.29 | 28 | – | CP |
J104912+575014 | 0.07256 ± 0.00002s | 127.26 | 0.60 | 45 | – | CP |
J105340+560950 | > 0.365 | 36.80 | 0.42 | 40 | 0.72 ± 0.05 | CP, SSC |
J105436+590901 | 0.8861 ± 0.0003s | 18.62 | 0.84 | 23 | – | CP |
J105524+561616 | 0.31 ± 0.03p | 26.93 | 0.29 | 39 | – | CP |
J103815+601111 | 0.19676 ± 0.00005s | 22.21 | – | – | > 0.80 ± 0.05 | SSC |
J103845+594414 | 0.38 ± 0.03p | 42.65 | 0.49 | 38 | 0.80 ± 0.05 | SSC |
J105057+562349 | 0.62 ± 0.07p | 6.71 | – | – | > 0.76 ± 0.05 | SSC |
J105418+595220 | 0.79 ± 0.04p | 24.65 | – | – | > 0.81 ± 0.05 | SSC |
J105723+565938 | > 1.1417 | 43.73 | > 0.34 | – | 1.1 ± 0.05 | SSC |
J102955+584621 | 0.39 ± 0.05p | 47.06 | < 0.09 | 46 | – | V |
J103621+564323 | 0.55 ± 0.05p | 579.19 | < 0.01 | 184 | – | V; DDRG |
J104252+553536 | 0.5221 ± 0.0002s | 50.03 | < 0.04 | 34 | – | V; DDRG |
J104809+573010 | 0.31742 ± 0.00007s | 38.82 | 0.15* | 24 | – | V |
J110021+601630 | 0.19857 ± 0.00003s | 294.30 | < 0.06 | 49 | – | V |
Notes. The columns show: source name of the candidate restarted radio source; photometric (p) or spectroscopic (s) redshift from the SDSS DR14 or lower limit redshift from the WISE W1 magnitude; the flux densities at 150 MHz from the 18″ catalogue in mJy (Mahony et al. 2016); the radio CP computed as described in Sect. 4.3.1; SB at 150 MHz; spectral index of the inner region and the selection methods used to identify the source (V = visual identification, CP = high core prominence, SSC = steep spectral index of the core).
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