Fig. 20
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Distribution of recalibration factors ℱ , derived by KVPIPE using the parameters provided by CASU, for VIKING and VIKINGlike observations in the KiDS+KiDZ fields. Following Driver et al. (2016) and Wright et al. (2019), we applied a rejection of detectors with recalibration factors ℱ ≥ 30. There are additional indirect selections, however, that occur for fields with large PSF sizes (see Sect. 6.4).
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