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Fig. 4.

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Magnitude errors vs observed apparent magnitudes for simulated LSST observations from the ELAIS N1 sample. Simulations are cut to the maximum LSST limit. The choice to vary simulation parameters allows us to obtain different errors for similar magnitude values, as we would expect in the case of real observations. The brightest end we reached is 13 mag, but for clarity of the plot, we cut it at 21 mag.

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