deletions | additions       diff --git a/figures/KIC_9246715_echelle_bis/caption.tex b/figures/KIC_9246715_echelle_bis/caption.tex  index 8f221d3..2ab1f4b 100644  --- a/figures/KIC_9246715_echelle_bis/caption.tex  +++ b/figures/KIC_9246715_echelle_bis/caption.tex 
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\label{fig:echelle} \'Echelle diagram of the power density spectrum presented in Figure \ref{fig:seismo}. Darker regions correspond to larger peaks in power density. The power density spectrum is smoothed by a boxcar over seven bins and cut into 8.31-$\mu\rm{Hz}$ chunks; each is then stacked on top of its lower-frequency neighbor. This representation allows for visual identification of the modes. \revise{Solid blue and dashed red lines \revise{Lines  are plotted to guide the eye on toward a theoretical  mode distribution according to the red-giant universal pattern \citep{mos11}. It is an indication on illustrates  how we expect the  modes are distributed to appear,  but is  not the result of a fitting. fit.  Solid blue and dashed red lines are associated with the main (nominally Star 2) and marginally-detected (nominally Star 1) oscillation set oscillations,  respectively. The variable $\ell = 0$ refers to the mode degrees. Large spacing is $\Delta\nu = 8.31\ \mu\rm{Hz}$ for the  main set (blue) lines  and $8.60\ \mu\rm{Hz}$ for the  secondary set (red) lines  (see Section \ref{subsubsec_second_osc}).}