Table 3.
Flux densities and map properties of the analysed sample.
| Galaxy | Ellipse a × b(a) | SHBA | σHBA | SL-Band | σLband |
 |
 |
|---|---|---|---|---|---|---|---|
| [arcmin2] | [Jy] | [μ Jy/Beam] | [Jy] | [μ Jy/Beam] | [kpc] | [kpc] | |
| NGC 891 | 5.9 × 4.55 | 3.3±0.3 | 207 | 0.68±0.03 | 31 | 28.4 | 15.6 |
| NGC 3432 | 4.35 × 2.2 | 0.30±0.03 | 165 | 0.086±0.004 | 22 | 14.4 | 8.5 |
| NGC 4013 | 2.36 × 1.45 | 0.151±0.015 | 167 | 0.0381±0.0019 | 34 | 16.1 | 5.4 |
| NGC 4157 | 4.25 × 2.08 | 1.01±0.10 | 196 | 0.180±0.009 | 35 | 34.8 | 21.7 |
| NGC 4631 | 8.8 × 7.5 | 4.46±0.45 | 235 | 1.03±0.05 | 25 | 30.0 | 24.6 |
Notes. We list the integrated flux density measurements in HBA (SHBA and L band (SL-Band), based on the described aperture, accounting for background noise (σHBA & σL-Band) as well as calibration errors. Physical diameters, based on the 3σ contours in HBA, parallel (
) and orthogonal (
) to the galactic disk are also listed.
Ellipses are defined in Heesen et al. (2022b) and encompass the 3σ contours of the re-calibrated LoTSS map.
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