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Fig. D.1


Comparison between synthetic spectra based on the spectroscopic temperatures (full blue lines) and temperatures from microlensing techniques (dashed red lines) to the observed Hα line profiles at 6563 Å for the 33 new stars. The stars are sorted by metallicity. Similar plots can be found for the other 58 stars in Bensby et al. (2011a, 2013).

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