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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.

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