deletions | additions       diff --git a/figures/visibility_mosser_suppressed_band/caption.tex b/figures/visibility_mosser_suppressed_band/caption.tex  index 3cdc258..c84aa05 100644  --- a/figures/visibility_mosser_suppressed_band/caption.tex  +++ b/figures/visibility_mosser_suppressed_band/caption.tex 
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\label{fig:moneyplot} Normalized visibility $V^2$ of $\ell=1$ modes as a function of $\nu_{\rm max}$. The star and circle  symbols represent data from \cite{Mosser_2011} normalized by 1.54 such that the average visibility of $\ell=1$ modes in non-suppressed oscillators is $V^2=1$ \cite{Ballot_2011}. Suppressed oscillators (orange stars) are identified following the same criteria as in \cite{Mosser_2011}. The theoretical band shows the visibility of dipole modes suppressed in a $1.6\,M_\odot$ star, as predicted by Eq.~\ref{eqn:vis}. The theoretical result is quite insensitive to the mass of the model. The visibility of the suppressed dipoles in KIC 8561221 \cite{Garcia_2014} and KIC 9073950 is also shown (diamond and circle symbols, respectively). Here we used values for $\tau$ in the range 5-20 days, consistent with \cite{Dupret_2009,Corsaro_2015}.