Table 3
Flux ratios of bright sources within snapshot from Obs. 3.
| Source | S60 | σ S 60 | Calibrated | σ | Ratio | Comment | |
| (Jy) | (Jy) | flux (Jy) | (Jy) | ||||
|
|
|||||||
| 3C 10 | 367.9 | 18.81 | 397.02 | 67 | 1.08 | VLSS Ng = 4, α = − 0.7 | |
| 3C 452 | 152.2 | 10.99 | 184.52 | 28 | 1.21 | VLSS Ng = 2, α = − 0.7 | |
| 3C 390.3 | 99 | 6.00 | 121.89 | 35 | 1.23 | VLSS Ng = 3, α = − 0.7 | |
| 3C 380 | 156.2 | 2.99 | 156.2 | 38 | 1 | (Scaife & Heald 2012) | |
| 3C 295 | 134.5 | 8.31 | 95.23 | 37 | 0.71 | (Scaife & Heald 2012) | |
Notes. The S60 flux has been derived from the best available modeled spectra, or −0.7 otherwise. Ng is the number of Gaussian components in the source. The calibrated flux ratio is derived after imaging the calibrated visibilities and generating lightcurves of peak flux from sources in the snapshots.