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Fig. 3.

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Spectrophotometry of the planet, normalized to d = 10 pc, compared to the best-fit model from HADES (red line). The black circles show the GPI spectrum, the blue square shows SPHERE photometry, and the green arrow indicates the SPHERE-IFS 5σ upper limit (all with 1σ errors). The orange line shows 5σ IFS upper limits in individual λ slices. The predicted photometric points are shown with red markers.

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