deletions | additions       diff --git a/MAYBE_REMOVE_NEXT_PARAGRAPH_AND__.tex b/MAYBE_REMOVE_NEXT_PARAGRAPH_AND__.tex  index 47ff659..499ad92 100644  --- a/MAYBE_REMOVE_NEXT_PARAGRAPH_AND__.tex  +++ b/MAYBE_REMOVE_NEXT_PARAGRAPH_AND__.tex 
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37 months of the Kepler mission. Our analysis is restricted to stars with \numax\   larger than 50\muhz\ and masses below 2.1\msol, which ensures it includes only red   giants that do not burn helium in their cores \citep{Stello_2013,Mosser_2014}.   %The missing dipole modes in a significant fraction of stars revented us using   %the dipole mode period spacings to select stars in this particular evolution stage  %\citep{Bedding_2011}.   %A comparison with lists of helium core burning stars based on measured period   %spacing \citep{Stello_2013,Mosser_2014} revealed only X stars in common with our   %sample. They all had \numax\$ < 70\,$\muhz.  It is striking how the stars form two distinct branches that gradually merge as the stars  evolve towards lower \numax. % This trend is also evident in Fig.1.   Most stars fall on the ``normal'' upper branch of visibilities around 1.5 in