Corrected dust-mass opacity in the LMC: histogram of extinction-corrected dust-mass opacity (κ₁₆₀) values for all ISM regions measured in the LMC. Compared to existing literature measurements of κ₁₆₀, both in the LMC and SMC (e.g., K. D. Gordon et al. 2014, 2017; J. Roman-Duval et al. 2017) and beyond (e.g., M101, 22 other galaxies; C. J. R. Clark et al. 2016; I.-D. Chiang et al. 2018, respectively), these new inferred measurements span broader values (κ₁₆₀ = 0.3–6 m² kg⁻¹). This discrepancy can be explained by the fact that the observed fields probe a wide range of ISM environments (Σ_H = 4–100 M_⊙ pc⁻²), especially compared to previous surveys that are often biased by measuring κ_D toward brighter, higher column-density regions of galaxies.