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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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