Fig. B.3.
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Comparison between the number of QSO candidates (blue) per magnitude bin in the EDF-N for the new Euclid-only colour cut, JH_IEY. In grey we show all Euclid compact sources in the corresponding magnitude bin. As the magnitude bins progress from brighter colours (left plot) to fainter (right plot), the number of sources and QSO candidates increases accordingly.
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