Table 2.
Information about the number of sources in the LS and its various parts.
| AGN | non-AGN | |||||
|---|---|---|---|---|---|---|
| Type I | Type II | MIR | X-ray | Stars | Gal | |
| spec-MIR LS (358 AGN) | 209 | 96 | 203 | – | 841 | 955 |
| c | (53 MIR-only) | |||||
| main LS (520 AGN) | 209 | 96 | 203 | 477 | 841 | 955 |
| (53 MIR-only) | (162 X-ray only) | |||||
Notes. The table shows the composition of the LS for the two parts of this work: the top line refers to the LS where we did not include AGN selected via their X/O, while these sources are included in the bottom line. The rest of the LS is unchanged and, in particular, the number of non-AGN in each LS is always 1796. The various columns indicate (left to right): AGN classified via optical spectroscopy as Type I or Type II, AGN selected via their MIR properties, AGN selected via their X/O, plus stars and inactive galaxies which make up the non-AGN part of the LS.
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