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Fig. 6

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Teff against spectral type for stars with luminosity class I. The blue dots correspond to stars with revised classifications (see Sect. 4.3), whereas the gray dots correspond to stars whose classification corresponds to the default provided by SIMBAD. The dashed orange and cyan lines correspond to a first- and third-order polynomial fit to the stars in blue. Some previous calibrations from the literature are also included for comparison.

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