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Table 6.
Percentage of AGNs and composites and star-forming galaxies with X-ray emission selected using MIR and near-IR methods according to the MEx criteria.
| Type | L04 | Ch17 | S05 | M12 |
|---|---|---|---|---|
| AGNs | 79% | 71% | 79% | 75% |
| Composites | 11% | 12% | 12% | 8% |
| SFs | 10% | 17% | 9% | 17% |
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