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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.