Differential source counts from MALS, uncorrected (beige circles) and corrected with completeness (purple hexagons) taking into account whether a source is resolved or unresolved. Lastly, source counts are also corrected with RMS noise coverage (green squares), which for the lowest flux bins goes to zero, causing solutions to diverge. This is all compared to the SKADS source counts, both for the central frequency of 1270 MHz (black), and for the full frequency range (grey area), and to the source counts derived from the MeerKAT DEEP2 image and NVSS from Matthews et al. (2021, white diamonds). The number counts are tabulated in Table 3.