deletions | additions       diff --git a/figures/KIC11725564_SiB_comparison_1/caption.tex b/figures/KIC11725564_SiB_comparison_1/caption.tex  index b66b02b..f39f425 100644  --- a/figures/KIC11725564_SiB_comparison_1/caption.tex  +++ b/figures/KIC11725564_SiB_comparison_1/caption.tex 
...
\label{fig:twin}  \textbf{THIS IS A PLACEHOLDER VERSION} Power density spectrum of KIC 11725564 (gray), a seismic ``twin'' of KIC 9246715 (red). Both power spectra were are  smoothed with a boxcar of 1/10 $1/10$  of the large separation. The modes in KIC 11725564, a secondary red clump star, have $\Delta \nu$ and $\nu_{\rm{max}}$ which very nearly match KIC 9246715. They are less noisy and have larger amplitudes than KIC 9246715, making this star a useful asteroseismic comparison.