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Table 2.
Percentage of AGNs and composite and star-forming galaxies selected using the MIR and near-IR methods according to the KEx criteria (Zhang & Hao 2018).
| Type | L04 | Ch17 | S05 | M12 |
|---|---|---|---|---|
| AGNs | 33% | 56% | 34% | 53% |
| Composites | 49% | 30% | 52% | 34% |
| SFs | 18% | 14% | 14% | 13% |
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