Comparison of the CO₂ and H₂O luminosities derived for CX Tau (green and blue stars, respectively) to the data shown in Banzatti et al. (2020) (shown in gray). The left panels show the H₂O and CO₂ luminosities as a function of accretion luminosity. The right panels show the H₂O and CO₂ luminosities corrected for the correlation with accretion luminosity as a function of dust radius. The reported correlation between the H₂O luminosity and the dust radius from Banzatti et al. (2020) is shown in the top panel, and the median CO₂ luminosity is shown in the bottom panel (both shown in a gray dashed line). We note that the measurements from our data on both plots contain 1σ error bars, but these do not exceed the marker size in the left panel.