Interquartile ranges (IQRs) for the log ratio of stellar A_Vs at different viewing angles, ﹩{{A}_{{\rm{V}}}}_{\theta ,\phi }﹩, and a function of the median extinction ﹩\widetilde{{A}_{{\rm{V}}}}﹩, shown for three different times in the simulation. Shown in red is the one-to-one line where ﹩{{A}_{{\rm{V}}}}_{\theta ,\phi }﹩ is equal to ﹩\widetilde{{A}_{{\rm{V}}}}﹩, while the blue shaded region shows inner quartile range. The histograms above are the number density of stars at a given ﹩\widetilde{{A}_{{\rm{V}}}}﹩ at that time, showing how many stars are contributing to the IQR.