Table 1.
[NeV] emitters vs. other AGN selection techniques.
| Sample | N | N in W1 | N X-ray AGN (%) | N MIR-AGN (%) | N MEx AGN (%) | N BBPT AGN (%) |
|---|---|---|---|---|---|---|
| Blue [NeV] | 269 | 200 | 11 (5.5 ± 1.7) | 9 (4.5 ± 1.5) | 24 (9 ± 2) | 21 (8 ± 2) |
| Blue parent | 5272 | 3552 | 47 (1.3 ± 0.2) | 33 (0.9 ± 0.2) | 112 (2.0 ± 0.2) | 67 (1.3 ± 0.2) |
| Green [NeV] | 95 | 62 | 1 (1.6 ± 1.6) | 1 (1.6 ± 1.6) | 4 (4 ± 2) | 4 (4 ± 2) |
| Green parent | 2636 | 1708 | 13 (0.8 ± 0.2) | 7 (0.4 ± 0.2) | 12 (0.5 ± 0.1) | 10 (0.4 ± 0.1) |
| Red [NeV] | 157 | 120 | 1 (0.8 ± 0.8) | 0 (0.0) | 0 (0.0) | 0 (0.0) |
| Red parent | 5272 | 3501 | 11 (0.3 ± 0.1) | 5 (0.14 ± 0.06) | 0 (0.0) | 0 (0.0) |
Notes. X-ray AGN: X-ray detected sources with X-ray luminosities greater than 1042 ergs s−1 or with NH ≥ 1022 cm−2. MIR-AGN: sources with 5σ detections at 3.6 μm and 4.5 μm and with S(4.5 μm)/S(3.6 μm) ≥ 1.27 (Stern et al. 2012). MEx AGN: sources with more than 3σ Hβ and [OIII] equivalent widths and EW([OIII])/EW(Hβ) ratios satisfying the MEx AGN selection criterion defined in Juneau et al. (2011). BBPT AGN: sources with more than 3σ Hβ, [OII], and [OIII] equivalent widths and EW([OIII])/EW(Hβ) and EW([OII])/EW(Hβ) ratios satisfying the blue BPT criterion defined in Lamareille (2010).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.