Comparison between the instantaneous SFR, the stellar mass (M_★), the dust mass (M_dust), and sSFR derived from GalaPy (G; y-axes) and CIGALE (C; x-axes). GMCs are color-coded following the legend at the middle panel. All fits were performed on log-transformed data, except for the SFR, which was fitted using the linear scale. Linear regression was initially performed using the linregress function from the SciPy package (Gommers et al. 2025), followed by Bayesian inference through Markov chain Monte Carlo (MCMC) sampling implemented in the emcee package (Foreman-Mackey et al. 2013).