deletions | additions       diff --git a/figures/emission_star3/caption.tex b/figures/emission_star3/caption.tex  index d5ffa43..021183a 100644  --- a/figures/emission_star3/caption.tex  +++ b/figures/emission_star3/caption.tex 
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\label{fig:emission1} Top of each panel: observed FDBinary extracted spectrum of Star 1 in KIC 9246715 (red) together with a stellar template (dotted black line). Bottom of each panel: difference between the model and observed spectra. Vertical lines show the position of each absorption line. Net emission in the Fe I lines indicates the likely presence of Zeeman splitting \citet{har73}. \citep{har73}.  Emission in the H$\alpha$ and Ca II lines are characteristic of chromospheric magnetic activity, and the presence of an He I absorption line indicates an upper chromosphere ($T > 10000 \ \rm{K}$) is present \citep{fro12}.