deletions | additions       diff --git a/SETTING_UP_FOR_THE_PRESENTATION__.tex b/SETTING_UP_FOR_THE_PRESENTATION__.tex  index d168b24..aba7ee9 100644  --- a/SETTING_UP_FOR_THE_PRESENTATION__.tex  +++ b/SETTING_UP_FOR_THE_PRESENTATION__.tex 
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%than for the radial modes ($V^2\simeq 1.5$)   \citep{Ballot_2011,Mosser_2011},  the stars with suppressed modes have $V^2\sim 0.5$ for \numax\ $\simeq 70\,$\muhz\ and   down to almost zero for the least evolved red giants oscillating above $200\,$\muhz. $200\,$\muhz\ (Fig. 1).  % a phenomena previously observerved in X red giants  % [refMosser2012LargeKepler] and a subgiant star [ref Droopy].