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Fig. 3
Top panel: lightcurve of an AGN candidate (ID 4362). Bottom panel: lightcurve of a supernova (ID 19508). The error bars do not represent the formal photometric error except the ⟨ σ ⟩ + 3 × rms⟨ σ ⟩ variability limit and are shown to allow the reader to visualise the significance of the variability.
This figure is made of several images, please see below:
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