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Table 1.

Summary table of the number of sources in each multi-wavelength catalogue and the different subsets explained in Sect. 3.

Catalogue Number Comments
eFEDS main 27 021* * = cut to eFEDS MOC texp > 500 s
LS DR9 11 255 466* Duplicate (“DUP”) sources removed
LOFAR 36 631* 24 613 compact, 12 018 complex
GAMA09 48 190 SC ≥ 6; z < 0.4; 21 462 mass-complete

eFEDS-LS9 20 696 Salvato et al. (2022); p_any > 0.035, CTP_quality > 2
eFEDS-LS9-GAMA09 584

LOFAR-LS9 22 759 (a) p_any > 0.06, S/N > 5; 16130 compact, 6629 complex
LOFAR-LS9-GAMA09 2619 (b) 1901 compact, 718 complex

GAMA09 (G9) X-ray AGN 523 325 mass-complete
G9 X-ray AGN in Quiescent gal. 147 124/147 mass-complete
G9 X-ray AGN in Star-forming gal. 376 201/376 mass-complete

G9 radio AGN 764 682 mass-complete (404/445 compact; 278/319 complex)
G9 radio AGN in Quiescent gal. 646 595/646 mass-complete (354/385 compact; 241/261 complex)
G9 radio AGN in Star-forming gal. 118 87/118 mass-complete (50/60 compact; 37/58 complex)

G9 radio + X-ray sources 121 74 (32)/92 mass-complete X-ray (radio) AGN; 24 radio + X-ray AGN

Notes.

(a)

The LOFAR-LS9 NWAY match yields 22 754 sources, to which 5 (out of 6) large FRII sources are added manually (the remaining large FRII source with LOFAR Source id 8153 was already present among the matched sources, albeit the optical CTP had to be corrected).

(b)

The mass-complete sources were visually inspected to confirm correct counterpart association and classify radio morphology. Two radio sources (LOFAR Source id: 10347, 27051) were found to be consistent with noise fluctuations of the background and are excluded from this point on (see more details in Appendix C).

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