Table 1.
VLA band L observations.
| Stokes I | Stokes V | ||||||
|---|---|---|---|---|---|---|---|
| Date | Time on-source | Peak | Integrated | σI | Peak | Integrated | σV |
| (dd/mm/yy) | (hours) | (mJy/beam) | (mJy) | (mJy/beam) | (mJy/beam) | (mJy) | (mJy/beam) |
| 21/01/18 | 6.1 | 3.77 ± 0.06 | 3.58 ± 0.10 | 0.05 | 1.49 ± 0.05 | 1.43 ± 0.08 | 0.04 |
| 20/02/18 | 5.7 | 2.79 ± 0.02 | 2.86 ± 0.04 | 0.02 | 0.54 ± 0.01 | 0.53 ± 0.02 | 0.01 |
| Combined | 11.8 | 3.25 ± 0.04 | 3.38 ± 0.07 | 0.03 | 1.02 ± 0.03 | 1.18 ± 0.05 | 0.03 |
Notes. The columns give the date, peak, and integrated fluxes of the source and the root mean square of the calibrated clean images, for Stokes I and V, for each observation and their combined image. The fluxes were calculated using the task imfit and performing a Gaussian fitting. The errors in the peak and integrated flux represent the statistical standard deviation from the Gaussian fitting.
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