Table 1.
QSO samples used in this study.
| Samples | LOFAR | SDSS | LOFAR |
|---|---|---|---|
| Fields | QSOs | 3σ detection | |
| ALLQSOs | Deep Fields + GAMA | 4436 | 2469 (56%) |
| Deep Fields | 2105 | 1555 (74%) | |
| GAMA | 2331 | 914 (39%) | |
| MWQSOs | Deep Fields + GAMA | 1789 | 1002 (56%) |
| Deep Fields | 480 | 451 (94%) | |
| GAMA | 1300 | 551 (42%) |
Notes. Description of the different samples used for this study, including the number of LOFAR detected quasars and their corresponding fractions. The MWQSOs and the ALLQSOs samples correspond to the areas in Figure 1 which are filled with grey stars and the light-cyan shaded areas, respectively.
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