Various properties measured for the CHIMPS clumps as functions of both Galactocentric (left column) and heliocentric distance (right column): (a) total clump mass; (b) volume-averaged number density (c) mean of the voxel column density distribution associated with the clump; (d) mean excitation temperature; (e) turbulent pressure; (f) virial parameter; and (g) heliocentric distance. In each case, the distribution of black points shows the full sample (described in Sect. 5), while the grey points show a heliocentric distance-limited subsample, lying between 8 ≤ d_k ≤ 12 kpc. The pink points show clumps from the distance-limited subsample that lie above the mass completeness limit at 12kpc. On the Galactocentric distance distributions, the blue trend lines show the mean values of clumps in 0.5 kpc-wide bins; while the orange trend lines show the same averages, but for the distance-limited subsample; and the thin red line shows the trend for the mass-complete distance-limited subsample. In the heliocentric-distance column, the dashed red lines denote approximate boundaries between the Bergin & Tafalla (2007) “cloud”, “clump”, and “core” definitions. The green curve in the M-d_k panel denotes the 90% completeness limit for compact sources, while the yellow shaded region denotes the parameter space below the 5σ survey sensitivity.