Notes. Column (1) displays the [C II]158 μm regions considered to compute the parameters. E^* and W^* represent the sum of all the [C II] clumps for each galaxy. Column (2) shows the clump correspondence between the regions identified in the ALMA rest-frame 160 μm and MIRIM F1000W images. The last two rows represent the total values for each galaxy, derived by summing all the clumps. Columns. (3)–(5) give the intrinsic dynamical, gas masses, and SFR derived from the [C II]158 μm ALMA spectral imaging (Spilker et al. 2022). Column (6) gives the extinction-corrected stellar masses derived from the MIRI F1000W imaging for a 50–100 Myr constant star formation presented in Table 4. Considering stellar populations created by a constant star formation of ∼10 Myr or instantaneous burst of 200–400 Myr would yield M_* different by a factor of ∼0.33 and ∼6.5, respectively. Columns. (7) and (8) show the ratio between the stellar mass computed in this work and the dynamical and gas masses derived from the [C II]. Column (9) displays the sSFR (SFR/M_*) derived using the SFR values computed by Spilker et al. (2022).