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Fig. 6
Top panel: differences in the temperature estimates by means of isochrone projection procedure and using the Alonso et al. (1999) relation (Δ(Tiso − TA99)) as a function of the Alonso et al. (1999) temperature (TA99) for all our target stars. Bottom panel: the same, but for the Alonso et al. (1996) calibration (TA96).
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