Fig. B.12.
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Application of the PCA correction to the example star Gaia DR3 604895948360165888 (panels a and b), and the fainter and essentially constant star Gaia DR3 604909310002693632 (panels c and d). Panels (a) and (c) each show the result of the instrumental systematics correction (blue) and the PCA correction (red) whereas panels (b) and (d) show the final light curve after the PCA correction was applied.
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