deletions | additions       diff --git a/We_quantify_the_mass_dependent__.tex b/We_quantify_the_mass_dependent__.tex  index b499c16..60689eb 100644  --- a/We_quantify_the_mass_dependent__.tex  +++ b/We_quantify_the_mass_dependent__.tex 
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We quantify the mass-dependent mode suppression in Fig. 3 by  showing the relative number ofsuppressed  stars with suppressed dipole modes  (those below the dashed line in Fig. 2) in narrow mass intervals.   We see no suppressed stars below 1.1\msun, while above this threshold there  is first a gradual increase followed by a rapid increase above approximately