Flux ratios of bright sources within snapshot from Obs. 3.
|Source||S60||σ S 60||Calibrated||σ||Ratio||Comment|
|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.