Dennis edited figures/histogram/caption.tex  almost 9 years ago

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Observed fraction of stars with suppressed dipole modes. The  abscissa is the stellar mass (in solar units) estimated from the seismic  scaling relations \citep{Stello2013}. \citep{Stello_2013}.  For each mass bin we calculated the suppressed star fraction as the number of stars that fall below the dashed line in  Fig. 2, relative to all stars in that same mass bin.   To make the distinction between normal and suppressed stars