deletions | additions       diff --git a/figures/visibility_mosser_suppressed_band/caption.tex b/figures/visibility_mosser_suppressed_band/caption.tex  index b16fa4a..bf8b224 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 function of $\nu_{\rm max}$. The star symbols represent data from \citet{Mosser_2011} normalized by 1.54 such that the average visibility of $\ell=1$ modes in non-suppressed oscillators  is $V^2=1$ \citep{Ballot_2011}. Suppressed oscillators (orange stars) are identified following the same criteria as in \citet{Mosser_2011}.  The theoretical band shows the visibility of dipole modes suppressed by the magnetic greenhouse effect in a $1.6\mso$ star, as predicted by Eq.~\ref{eqn:vis}. The theoretical result is quite insensitive to the mass of the model.Suppressed dipoles (orange stars) are identified following the same criteria as in \citet{Mosser_2011}.  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 $\tau_0$ in the range 5-20 days, consistent with \cite{Dupret_2009,Corsaro_2015}.