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Table 1.
Samples considered in this paper.
Name | Description | Number of objects |
---|---|---|
Full | Complete sample of Williams et al. (2019) | 318 520 |
FC | Flux-complete, flux cut at 0.5 mJy | 239 845 |
O | Optical ID exists | 231 716 |
FCO | Intersection of FC and O | 172 898 |
Z | Some redshift estimate exists | 162 249 |
ZG | “Good” photometric redshift exists | 89 671 |
FCOZG | Intersection of FCO and ZG | 71 955 |
FCOZGM | Cross-match of FCOZG with the MPA-JHU sample | 12 803 |
FCOZGM RLAGN | RLAGN selected from FCOZGM | 3706 |
FCOZGM SFG | SFG selected from FCOZGM | 9097 |
RLAGN | RLAGN selected from FCOZG | 23 344 |
SFG | SFG selected from FCOZG | 41 998 |
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