Table 1.
uGMRT observations.
| Stokes I | Stokes V | ||||||
|---|---|---|---|---|---|---|---|
| Date | Clean beam | Peak | Integated | σI | Peak | Integrated | σV |
| (dd/mm/yy) | (″ × ″) | (mJy/beam) | (mJy) | (mJy/beam) | (mJy/beam) | (mJy) | (mJy/beam) |
| 11/06/23 | 5.75 × 4.02 | 1.094 ± 0.017 | 1.076 ± 0.030 | 0.014 | 0.160 ± 0.010 | 0.183 ± 0.021 | 0.009 |
| 29/07/23 | 4.96 × 4.09 | 1.299 ± 0.014 | 1.217 ± 0.023 | 0.013 | 0.200 ± 0.009 | 0.188 ± 0.016 | 0.008 |
| Combined | 4.99 × 3.92 | 1.200 ± 0.013 | 1.190 ± 0.023 | 0.012 | 0.185 ± 0.007 | 0.183 ± 0.012 | 0.006 |
Notes. The columns give the date, clean beam size, peak, and integrated fluxes of the source and the rms of the self-calibrated clean images, for Stokes I and V, for each observation and their combined image. Each observation lasted 7 hours, including overheads. The fluxes were calculated using the task imxfit 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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