deletions | additions       diff --git a/SETTING_UP_FOR_THE_PRESENTATION__.tex b/SETTING_UP_FOR_THE_PRESENTATION__.tex  index 687d814..8484ff5 100644  --- a/SETTING_UP_FOR_THE_PRESENTATION__.tex  +++ b/SETTING_UP_FOR_THE_PRESENTATION__.tex 
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For ``normal'' stars (top panels), the observed integrated power in the dipole  modes (red peaks) is typically about 50-60\% larger than for the radial  modes (black peaks) as usual in Kepler observations [ref  Ballot2011/Mosser2012LargeKepler]. However, at each stage of evolution  we find stars with significantly suppressed dipole modes (bottom panels).  % a phenomena previously observerved in X red giants  % [refMosser2012LargeKepler] and a subgiant star [ref Droopy].