Table C.1.
Best-fit flux estimated from the dedicated radio observations of a sub-set of sources within the RACS sample.
| Source | Central Frequency | Flux | Flux error | Telescope |
|---|---|---|---|---|
| (GHz) | (mJy) | mJy | ||
| RACS J0036−37 | 2.1 | 0.67 | 0.13 | ATCA |
| 5.5 | 0.73 | 0.07 | ATCA | |
| 9.0 | 0.39 | 0.07 | ATCA | |
| RACS J0110−39 | 2.1 | 10.1 | 0.3 | ATCA |
| 5.5 | 5.3 | 0.4 | ATCA | |
| 9.0 | 3.7 | 0.2 | ATCA | |
| RACS J0127−44 | 2.1 | 13.7 | 0.2 | ATCA |
| 5.5 | 13.7 | 0.2 | ATCA | |
| 9.0 | 12.1 | 0.3 | ATCA | |
| RACS J0202−17 | 2.1 | 16.1 | 0.1 | ATCA |
| 5.5 | 19.1 | 0.1 | ATCA | |
| 9.0 | 13.8 | 0.1 | ATCA | |
| RACS J0209−56 | 2.1 | 13.0 | 0.2 | ATCA |
| 5.5 | 10.4 | 0.1 | ATCA | |
| 9.0 | 9.5 | 0.1 | ATCA | |
| RACS J0320−35 | 0.4 | 5.6 | 0.9 | uGMRT |
| 0.65 | 4.0 | 0.2 | uGMRT | |
| 2.1 | 2.09 | 0.09 | ATCA | |
| 5.5 | 0.84 | 0.03 | ATCA | |
| 9.0 | 0.63 | 0.03 | ATCA | |
| RACS J0322−18 | 0.4 | 4.0 | 0.3 | uGMRT |
| 0.65 | 2.5 | 0.1 | uGMRT | |
| 2.1 | 1.28 | 0.06 | ATCA | |
| 5.5 | 0.61 | 0.03 | ATCA | |
| 9.0 | 0.44 | 0.03 | ATCA | |
| RACS J1011−01 | 5.5 | 4.0 | 0.2 | ATCA |
| 9.0 | 2.7 | 0.2 | ATCA | |
| RACS J1322−13 | 5.5 | 53.27 | 0.2 | ATCA |
| 9.0 | 46.60 | 0.1 | ATCA | |
| RACS J1426−11 | 5.5 | 2.54 | 0.2 | ATCA |
| 9.0 | 1.6 | 0.1 | ATCA | |
| RACS J2020−62 | 2.1 | 0.82 | 0.20 | ATCA |
| 5.5 | 0.80 | 0.08 | ATCA | |
| 9.0 | 0.43 | 0.05 | ATCA | |
| RACS J2252−51 | 1.3 | 16.91 | 0.07 | MeerKAT |
| 2.2 | 15.43 | 0.05 | MeerKAT | |
| 3.1 | 12.30 | 0.04 | MeerKAT | |
| 2.1 | 16.1 | 0.2 | ATCA | |
| 5.5 | 6.7 | 0.1 | ATCA | |
| 9.0 | 4.0 | 0.1 | ATCA | |
| 5.5 | 6.51 | 0.05 | ATCA | |
| 9.0 | 3.65 | 0.03 | ATCA | |
Notes. Flux densities derived from dedicated observations of a sub-sample of the RACS high-z quasars. The errors reported here are the ones derived from the 2D Gaussian fit of the source in the given image and do not take the uncertainty in the flux scale calibration (assumed to be 5%) into account.
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