Table 1.
Subset of existing samples of X-ray selected AGN with spectroscopic redshift.
| Name | N | Area | X-ray |
References | ||
|---|---|---|---|---|---|---|
| (deg2) | Band | FXlim | ||||
| SPIDERS | 10 849 | 5128.9 | Soft | [−12.5,−12] | This paper | |
| XMM-XXL-N | 2578 | 18.0 | Both | [−15,−14] | B10, G17, Me16 | |
| Stripe 82X | 1886 | 31.3 | Both | [−15,−14] | A17, L19 | |
| X-Bootes | 2424 | 7.7 | Both | [−15,−14] | M05,K12 | |
| COSMOS | 2169 | 2.2 | Both | [−16,−15] | B10, S09, S11, Ma16, H18 | |
| AEGIS X | 354 | 0.3 | Both | [−17,−16] | N15 | |
| CDFS | 653 | 0.2 | Both | [−17,−16] | H14, L17 | |
| CDFN | 351 | 0.2 | Both | [−16.5,−15.5] | X16 | |
| LH | 115 | 0.2 | Both | [−16,−15] | F12 | |
Notes. The area covered is given in square degrees. The X-ray band signifies whether the sample was built using soft X-rays, hard X-rays or both. FXlim gives the range in which the flux limits of the samples are located. This is an order of magnitude, please refer to the articles to derive exact values.
References. M05: Murray et al. (2005), S09: Salvato et al. (2009), B10: Brusa et al. (2010), S11: Salvato et al. (2011), F12: Fotopoulou et al. (2012), K12: Kochanek et al. (2012), H14: Hsu et al. (2014), N15: Nandra et al. (2015), Ma16: Marchesi et al. (2016), Me16: Menzel et al. (2016), X16: Xue et al. (2016), A17: Ananna et al. (2017), G17: Georgakakis et al. (2017), L17: Luo et al. (2017), H18: Hasinger et al. (2018), L19: LaMassa et al. (2019).
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