Fig. 2
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Pixel-by-pixel spectroscopic light curves of HAT-P-55 observed with GTC/OSIRIS. First row: spectra of HAT-P-55 and the reference star. Second row: matrix of pixel light curves after removal of the common mode systematics. Third row: matrix of the best-fit light curve residuals. Fourth row: rms of each pixel light curve, compared to the expected photon noise.
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