Fig. A.11.
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Same as Fig. A.3, but for two candidates in Sample 2G-D of light curves modelled with only two Gaussians. The top set shows a case with a convincing primary eclipse detection while the secondary eclipse is spurious (Gaia DR3 2056622657089571968). The bottom set shows a seemingly good case from the G light curve (Gaia DR3 4077271415493214080).
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