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Table 4.
Number of AGNs selected based on the MIR features for the ELAIS N1 and COSMOS fields.
| Method | ELAIS N1 | COSMOS | Total sample |
|---|---|---|---|
| Stern et al. (2005) | 1269 (3.48%) | 1334 (9.50%) | 2603 (5.16%) |
| Donley et al. (2012) | 497 (1.36%) | 291 (2.08%) | 788 (1.56%) |
Notes. The last column shows the total number (and percentage) of AGNs in the full sample.
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