Fig. 8
Illustration to see how well the spectroscopic temperatures (full blue lines) and temperatures from microlensing techniques (dashed red lines) reproduce the observed wing profiles of the Hα line at 6563 Å for the 32 new microlensed bulge dwarfs. Note that no estimate of the temperature from microlensing techniques is available for OGLE-2011-BLG-1410S. The stars are sorted by metallicity.
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