Fig. 4
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CARMENES VIS, CARMENES NIR, and HIRES RV data for TOI-1801 (green, red, and blue dots, respectively). Top panel: combined model (black line) with its 1σ level of confidence (grey shadow), and Keplerian model for the planet (dashed orange line). Middle panel: Keplerian model alone (dashed orange line) after subtracting the best activity model. Bottom panel: residuals for the best-fit.
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