Table 2
Number of sources of: (1) selected sample; (2) SN candidates (see Sect. 5.1); (3) Candidates with X-ray detection (Hsu et al. 2014, see Sect. 5.2); (4) AGN candidates (AGN SED in Hsu et al. 2014, see Sect. 5.2); (5) Star candidates (diagnostic r−i versus 3.6 μm to r band flux ratios, see Sect. 5.3.1); (6) AGN Lacy et al. (2004) diagnostic using IR colours, see Sect. 5.3.2; (7) AGN candidates confirmed in optical spectroscopy by Boutsia et al. (2009) (BLAGN, Sect. 5.2).
| N | ||
|
|
||
| (1) | Selected | 175 |
|
|
||
| (2) | SN | 21/175 |
| (3) | X-rays | 12/15 |
| (4) | AGN (SED) | 12/15 |
| (5) | Stars (r, i, 3.6 μm) | 6/57 |
| (6) | AGN (IR) | 103/115 |
| (7) | AGN (spectra) | 9/9 |
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