Distributions of the MAGPHYS SED results and other physical parameters, shown separately for the spectroscopically confirmed sources (red histogram) and the sources with photometric redshifts (blue histogram). The panels from top to bottom, left to right, show the χ² (goodness of fit) values of the best-fit MAGPHYS SEDs, stellar masses, total-IR luminosities (the upper x-axis shows the corresponding L_IR-based SFRs), dust masses, dust temperatures, MAGPHYS-derived SFRs (Δt = 100 Myr), ratios between the L_IR-based SFR and that directly output by MAGPHYS, specific SFRs, starburstiness parameters (distance from the MS mid-line; see Sect. 4.1), and the ALMA 1.3 mm-based gas masses (Sect. 3.2). Base-10 logarithms are used for the masses, L_IR, and MAGPHYS-derived SFRs. The vertical dashed lines mark the full sample medians (see Table 1), and the additional red vertical line in the starburstiness panel shows the upper boundary of the MS (i.e. Δ_MS = 3, above which the source can be defined as a starburst galaxy).