Disk mass distributions in NGC 2024 East (dark blue) (left) and West (dark blue) (right) compared to disk masses in other SFRs. Data for the low-mass regions was taken from Barenfeld et al. (2016) for Upper Sco, Williams et al. (2019) for ρ Ophiuchi, Ansdell et al. (2016) for Lupus, and Cazzoletti et al. (2019) for Corona Australis. Disk masses across Orion are taken from Eisner et al. (2018) for the Trapezium, Ansdell et al. (2017) for σ Ori, and van Terwisga et al. (2019) for OMC-2. Silhouettes in the right panel show the low-mass regions Lupus, ρ Ophiuchi, and Upper Sco again, for comparison. The disk mass distributions for Class 0 and Class I objects across Orion from Tobin et al. (2020) are shown in dark- and light gray in both panels, using the same temperature (T_eff = 20 K) and opacity as the more evolved regions.