Table 5: Radio data used in the construction of the LTS source RLF. Column 1: spectral class or galaxy; Col. 2: number of relevant sources surveyed. In parentheses are the number of radio-detected sources. Please note that some sources may be in multiple radio surveys; Col. 3: observing frequency; Col. 4: resolution; Col. 5: instrument; Col. 6: flux limit (5$\sigma $); Col. 7: reference.
Class/   $\nu$ Res.   F $_{\rm limit}$  
Galaxy N (GHz) (mas) Instr. (mJy) Ref.
(1) (2) (3) (4) (5) (6) (7)
Seyfert 52 (37) 5 1000 VLA 0.2 1
LINER 45 (19) 15 150 VLA 1.0 2,3
  88 (37) 15 150 VLA 1.0 4
  52 (14) 5 100 MERLIN 0.5 5
Composite 39 (7) 15 150 VLA 1.1 2,3
  62 (9) 15 150 VLA 1.0 4
  16 (1) 5 100 MERLIN 0.5 5
  35 (26) 8.4 2500 VLA 0.3 6,7
NGC 660 ... 8.4 200 VLA 0.03 8
NGC 7331 ... 5 2000 VLA 0.1 9
REFERENCES - (1) Ho & Ulvestad (2001); (2) Nagar et al. (2002); (3) Nagar et al. (2000); (4) Nagar et al. (2005) and references therein; (5) this paper; (6) Filho et al. (2002a); (7) Filho et al. (2000); (8) data kindly provided by J. Ulvestad; (9) Cowan et al. (1994).

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