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Table 3

Statistics on the L20 cm/LHα (in logarithmic value) bins of the optical-radio sample to show the number of different objects placed in the Seyfert, LINER, or SF region (Figs. 2, 3), or AGN, composite, or SF region (Fig. 4) of the diagnostic diagrams.

Diagram Spectral type L20 cm/LHα < 0.702 0.702 < L20 cm/LHα < 0.708 0.708 < L20 cm/LHα < 0.716 L20 cm/LHα > 0.716

Seyferts 126 ± 11 (5.4%) 347 ± 19 (14.5%) 859 ± 29 (36.5%) 848 ± 29 (36.5%)
[Oi] LINERs 20 ± 5 (0.8%) 64 ± 8 (2.7%) 254 ± 16 (10.8%) 1162 ± 34 (50.0%)
SFGs 2199 ± 47 (93.8%) 1973 ± 44 (82.8%) 1241 ± 35 (52.7%) 315 ± 18 (13.5%)

Seyferts 88 ± 9 (3.7%) 261 ± 16 (10.9%) 676 ± 26 (28.7%) 722 ± 27 (31.0%)
[Sii] LINERs 10 ± 3 (0.4%) 24 ± 5 (1.0%) 136 ± 12 (5.8%) 842 ± 29 (36.2%)
SFGs 2247 ± 47 (95.8%) 2099 ± 46 (88.0%) 1542 ± 39 (65.5%) 761 ± 28 (32.7%)

AGNs 134 ± 12 (5.7%) 346 ± 19 (14.5%) 918 ± 30 (39.0%) 1570 ± 40 (67.5%)
[Nii] Composites 659 ± 26 (28.1%) 820 ± 29 (34.4%) 925 ± 30 (39.3%) 617 ± 25 (26.5%)
SFGs 1552 ± 39 (66.2%) 1218 ± 35 (51.1%) 511 ± 23 (21.7%) 138 ± 12 (5.9%)

Notes. The relative fraction of spectral types is reported in parenthesis.

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