Open Access
Table 1.
Main parameters of the radio images used in this work (see Fig. 2).
| Project ID/Survey | Telescope | νc [MHz] | Δν [MHz] | σ [Jy PSF−1] | PSF [″] | LAS [′] | Bmax [λ] |
|---|---|---|---|---|---|---|---|
| LT16_004/LoLSS | LOFAR | 54 | 24 | 1.4 × 10−3 | 15.0 | 210 | 16.1 × 103 |
| LC3_008/LoTSS | LOFAR | 144 | 47 | 57.4 × 10−6 | 6.0 | 66 | 41.2 × 103 |
| 36_020 | uGMRT | 383 | 200 | 23.1 × 10−6 | 8.7 × 6.8 | 32 | 31.9 × 103 |
| 36_020 | uGMRT | 650 | 200 | 6.6 × 10−6 | 4.7 × 3.4 | 17 | 54.2 × 103 |
| APERTIF | WSRT | 1365 | 130 | 70.4 × 10−6 | 33.1 × 30.0 | 10 | 6.8 × 103 |
Notes. (3) Central frequency; (4) Bandwidth; (5) Image noise; (6) Image resolution, arc-seconds; (7) Largest angular scale to which the instrument configuration is sensitive (arc-minutes); and (8) Maximum baseline length (wavelengths).
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.