Fig. 13
RFI levels and variances as a function of the time of day. The RFI percentages are smoothed. Although there is some variation in the detected RFI during the observation, this is likely not because of a different occupation of RFI between day and night. Instead, they are likely caused by the changing sky, since they correlate with the variance of the data and visual celestial artefacts in the dynamic spectra.
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