Table 5.
Details on the polarisation images.
| Resolution | Bandwidth | Channel width | Number of channels | Map noise | max Faraday depth | Faraday resolution | max recovered scale | ||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| Θ [″] | Δν [GHz] | δν [MHz] | σrms [μJy beam−1] |
||ϕmax|| [rad m−2] | δϕ [rad m−2] | Δϕmax [rad, m−2] | |||||
| L band | S band | I | Q | U | P | ||||||
| 5 | 2.0–4.0 | 8 | – | 168 | 6.4 | 4.7 | 4.7 | 9.9 | 1400 | 205 | 558 |
| 12.5 | 1.34–4.0 | 8 | 41 | 155 | 21.5 | 11.5 | 11.0 | 23.4 | 1400 | 78 | 558 |
Notes. Column 1: Observing resolution. Column 2: Observing bandwidth (i.e. first and last frequency channels). Column 3: Single-channel width. Column 4: Number of channels for the L and S band. Column 5: Map noise for the Stokes I, Q, and U calculated as the standard deviation of the datacube and for the total averaged polarised intensity P (not corrected for the Ricean bias). Column 6: maximum observable Faraday depth. Column 7: Resolution in the Faraday space. Column 8: Resolution in the Faraday space. Column 9: Largest observable Faraday scale.
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