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Table 2.
Assumed values for the radio observing parameters considered in this work: central observing frequency, beam resolution, thermal rms noise per beam, and detection threshold considered in our analysis (considering a 3σ detection, also including confusion noise).
| Telescope | Frequency | Beam | σrms | Detection thr. |
|---|---|---|---|---|
| (MHz) | (″) | (μJy beam−1) | (μJy arcsec−2) | |
| SKA-LOW | 260 | 7.3 | 4.8 | 0.24 |
| LOFAR-HBA | 120 | 25 | 250 | 1.05 |
| MWA Phase I | 200 | 120 | 10 000 | 1.83 |
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