Median dust attenuation curves for our full galaxy sample binned in terms of key parameters: (left panel) V-band attenuation (A_V), and (right panel) mass-weighted stellar age (⟨a⟩_*^m). The median attenuation curves are plotted as solid lines, and the shaded regions indicate their 1σ dispersion. These curves and uncertainties were estimated using a bootstrapping approach, where 5000 synthetic curves were generated and the 16th, 50th, and 84th percentiles were taken from the resulting distribution. For comparison, the Calzetti, MW, and SMC empirical curves are displayed as solid, dashed, and dotted black lines, respectively. The bin limits were chosen to maintain a roughly equal number of sources per bin (∼40 − 50 sources in four bins).