Table 1
Classification definitions of NELG objects.
| Sub-sample | Optical1 | X-ray1 | N | T ≥ 10 | X/O ≥ 0.1 | FWHMHβ > 600 km s-1 | |
| % | % | % | |||||
|
|
|||||||
| BPT-SF | true-SF | SF | SF/AGN | 38 | 0.10 | 0.00 | 0.03 |
| missing-AGN | SF | AGN | 28 | 0.93 | 0.96 | 0.89 | |
| BPT-AGN | weak-AGN | AGN | SF/AGN | 62 | 0.03 | 0.08 | 0.05 |
| strong-AGN | AGN | AGN | 83 | 0.30 | 0.79 | 0.19 | |
Notes. Column 1: sub-sample name; Col. 2: classification of the source using the Kauf03’s line as a separation criterion between SF and AGN activity; Col. 3: X-ray based classification according to hard X-ray luminosity, LX; Col. 4: total number of sources in the subsample; Col. 4(5): the fraction of sources in the subsample that display a thickness parameter (X-ray-to-optical flux ratio) higher than 1 (0.1) as expected for a typical AGN; Col. 5: the fraction of sources that exhibit an HβFWHM larger than 600 km s-1.
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