Fig. 1
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Comparison of the distribution of the effective temperature in our sample of Am and Fm stars for different modules in Gaia DR3. The GSP-Phot module is shown in blue in all three panels. Orange: assumption of binary star system. Green: assumption of hot star (Teff > 7500 K). Red: Same assumptions as GSP-Phot, but using medium resolution spectroscopy instead of photometry.
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