Table 4
Parameters of the SVC mosaics.
| Field | Date of observation (dd-mm-yyyy) | RA(a) (hh:mm:ss) | Dec (a) (dd:mm:ss) | σPI(b) (µJy beam–1) | FWHMPI (″) | σTP(b) (µJy beam–1) | FWHMtp (″) |
|---|---|---|---|---|---|---|---|
| SVC1 | 09-04-2019 | 22:48:39 | +33:56:40 | 14 | 32.1 × 18.0 | 35 | 27.2 × 12.1 |
| SVC2 | 09-04-2019 | 14:03:24 | +53:24:05 | 13 | 19.3 × 14.6 | 43 | 18.6 × 12.8 |
| SVC3 | 10-04-2019 | 01:55:19 | +33:56:40 | 14 | 29.2 × 16.1 | 42 | 26.2 × 11.7 |
| SVC4 | 11-04-2019 | 22:46:24 | +38:48:32 | 16 | 24.8 × 14.8 | 39 | 23.7 × 12.0 |
| SVC5 | 11-04-2019 | 14:15:53 | +36:22:36 | 16 | 3l.2× 17.7 | 46 | 25.5 × 11.9 |
Notes. (a)Coordinates correspond to the telescope pointing positions. (b)σΡΙ and σTP are the noise levels of the polarised intensity and total power images, respectively, which were derived by determining the lowest quartile of the pixel values of the corresponding rms maps from the PyBDSF source finding.
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