Table 1.
Accuracy and fraction of outliers obtained for X-ray surveys at different X-ray depths.
| Survey | Flux limit | Area | Photometry | Accuracy | Fraction of outliers | Method |
|---|---|---|---|---|---|---|
| Ref. | erg/s/cm2 | deg2 | σNMAD | η | ||
| Chandra-COSMOS | 1.9 × 10−16 | 0.9 | N/I/B, Uv-O-NIR-MIR | 0.015 | 6% | SED fitting |
| (Salvato et al. 2009) | ||||||
| XMM-COSMOS | 1.17 × 10−15 | 2.13 | N/I/B, Uv-O-NIR-MIR | 0.015 | 6.3% | SED fitting |
| Salvato11 | ||||||
| CDFS | 9.1 × 10−18 | 0.13 | N/I/B, Uv-O-NIR-MIR | 0.014 | 6.7% | SED fitting |
| (Hsu et al. 2014; Luo et al. 2010) | ||||||
| Stripe 82X XMM archival | 7 × 10−17 | 7.4 | B, UV-O-NIR-MIR | 0.06 | 13.2% | SED fitting |
| (Ananna et al. 2017) | ||||||
| Stripe 82X (XMM archival) | 7 × 10−17 | 7.4 | B, UV-O-NIR-MIR | 0.06 | 12.7% | ML |
| (Brescia et al. 2019) | ||||||
| Stripe 82X (XMM archival) | 1 × 10−14 | 7.4 | B, UV-O-NIR-MIR | 0.122 | 13.1% | ML |
| (Brescia et al. 2019) | ||||||
| XMM-SERVS | 1 × 10−14 | 4.5 | B, Uv-O-NIR-MIR | 0.04 | 9.2% | SED fitting |
| (Ni et al. 2021) | ||||||
| XMM-SERVS | 1.3 × 10−14 | 3.0 | B, Uv-O-NIR-MIR | 0.04 | 9.6% | SED fitting |
| (Ni et al. 2021) | ||||||
Notes. Modified version of the table presented in Ananna et al. (2017). The X-ray flux is measured in the 0.5–2 keV range (0.5–10 keV for XMM-SERVS). In addition, we report the area coverage, type of photometry available (narrow, intermediate, broadband photometry), and wavelength coverage (UV, Optical, NIR, MIR).
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