They are associated. In theory, DM because there is more of it, clumped first. And concentrations of DM helped to pull ordinary matter (OM) together by its gravity, leading to regions of higher than average density of OM.
So there is a correlation---regions where there is higher than average density of DM tend also to have pockets of higher than average density OM---not just visible in the form of stars but also gas, dust etc.
But the correlation wouldn't be absolute. there would be regions containing SOME dark matter, maybe just at very low density, in which no significant amount of OM had collected.
I'd be interested to see some of those maps, if you happen to have links to some online ones. DM is hard to detect except where it is in unusually high concentration and there are steep gradients in density that cause an optical distortion of the background (gravitational lensing). I wouldn't expect most DM to register that way---it would be too uniformly spread out. Maybe they just don't show DM where it is below a certain density. Anyway I'm wondering how the maps were made.