Table 3.
OTELO sources at z ∼ 0.4 and fraction of emitters and AGNs.
Objects at | Hα | AGNs | ||
---|---|---|---|---|
z ∼ 0.4 | Emitters | Optical | X-rays | Total |
∼186 | 46 | 12 | 1 | 13 |
100% | ∼25% | ∼7% | ||
100% | 26% |
Notes. First column: total number of OTELO sources at z ∼ 0.4 (see text for details). Second column: total number of Hα selected emitters. Third and fourth columns: number of optically selected and X-rays-selected AGNs at that redshift. Fifth column: total number of AGNs at that redshift. The second row shows the proportion of emitters and AGNs over the total sample of objects at that redshift. The third row indicates the proportion of optically selected AGNs (NLAGNs or BLAGNs) over the sample of emitters. Due to the small numbers that are being managed here, and the uncertainty in the estimation of the total number of sources at z ∼ 0.4, these numbers, especially those in the second row, should be taken with caution.
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