deletions | additions       diff --git a/figures/vis_vs_numax2/caption.tex b/figures/vis_vs_numax2/caption.tex  index c8c8c10..3a79902 100644  --- a/figures/vis_vs_numax2/caption.tex  +++ b/figures/vis_vs_numax2/caption.tex 
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Visibility of dipole modes for red giants observed with Kepler. The abscissa is the central frequency of the oscillations, which correlate closely with surface gravity shown at the top axis. Stars evolve from right to left in the diagram, corresponding roughly to the beginning of the red giant phase to the red giant luminosity bump \citep{Salaris_2005}. Each panel shows stars in a different mass bracket increasing from top to bottom (indicated by the colour bar annotation on the right). Mass is calculated from asteroseismic scaling relations \citep{Stello_2013}, and has a formal uncertainty below 10\% \citep{Miglio_2011}. The solid black line shows the theoretical predicted visibility of suppressed dipole modes (Fuller et al. 2015) assuming a mode lifetime for radial modes of 20 days \citep{E_Corsaro_2015}. The fiducial dashed line separates the two branches of normal and suppressed dipole-suppressed  stars.