Table 2.
Number of sources satisfying each selection criteria that resulted in the selection of candidate restarted galaxies.
No. | % | |
---|---|---|
FRI+FRII RLAGNs sample in BM19 | 1679 | |
Core-D AGNs sample in BM19 | 99 | |
Small-unreliable (excluded) | 5 | |
Core-D AGNs sample used | 94 | |
LOFAR 18″ detections | 94 | 100 |
LOFAR 6″ core detections | 94 | 100 |
FIRST core detections | 81/94 | 86 |
NVSS detections | 79/94 | 84 |
FIRST core and NVSS detections | 77 | |
CP1.4 GHz + SB144 MHz | 73 | |
SSC144 MHz, 1.4 GHz ≤ −0.65 | 15 | |
USSext (< − 1.2) + bright core | 9 | |
Morphology | 0 | |
Type-1 AGNs | 10 | |
Type-1 AGNs + USS | 2 | |
Type-1 AGNs (excluded) | 8 | |
One-sided jet morphology (excluded) | 2 | |
No. of candidate restarted galaxies | 69 |
Notes. For more details, readers can refer to Sect. 3. Acronyms: CP – high radio core prominence at 1.4 GHz, SB – surface brightness at 144 MHz; SSC – steep spectrum core; USS – ultra-steep spectrum of the extended emission. BM19 stands for Mingo et al. (2019).
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