[OII] line and CO luminosities (respectively left and right panels for each galaxy) in position-velocity planes corresponding to the DEEP2 slits. Smoothed ensembles of clumps are separated by eye along the vertical axis, as shown with the white horizontal lines. The [OII] diagrams were normalized in order to have fluxes proportional to the SFR, but all galaxies share the same arbitrary color scales. One arcsecond corresponds approximately to 8.5 kpc (Table 1).