Clustering strength, as a function of number density, split by galaxy type, with passive galaxies shown in the left hand panel and star-forming galaxies in the right hand panel. In both panels, the coloured symbols show the results for the WIRDS data, whilst the lines show the predictions from galform. The grey symbols show results from the literature, with the z = 0.3,0.5,0.7 LRG results from Sawangwit et al. (2011, large open circles), the z = 0.7,1.0 LRG results from Nikoloudakis et al. (2013, small open circles) and the passive (plotted left) and star-forming (plotted in the right panel) z = 1 results of Coil et al. (2008, filled squares in both panels).