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Fig. 16

Fig. 16 Refer to the following caption and surrounding text.

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Contrast curve and mass limits for the SHARK-NIR (blue) and LMIR-Cam (orange) observations of HD 128717 conducted on the night of May 16, 2025 UT. Top panel: contrast curve. Bottom panel: mass limits, with the thick curve corresponding to the nominal 1.40 Gyr stellar age and the shaded region to the age uncertainty.

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