Clustering using Galform in the ghsmc_800 simulation

I've populated the ghsmc_800 simulation (800³ particles, 480Mpc/h, σ₈=0.74, Ω_m=0.236, Ω_Λ=0.764, n=0.95) with output from the new version of Galform, using the models of Cole et al. (2000), Baugh et al. (2005) and Bower et al. (2006), and with output from the old version of Galform, using the models of Cole et al. (2000), Cole et al. (2000) with a higher baryon fraction, and 'Model M'. The plots below compare the clustering in these models and the clustering of the dark matter to clustering from the SDSS and 2dFGRS.

SDSS

The projected correlation function (actually r_pw_p(r_p)) for samples with a space density n_g/(h³ Mpc^-3) of 0.00117, 0.00308 (the fiducial space density from Harker, Cole & Jenkins 2007) and 0.01015:

Old Galform	New Galform
0.00117	0.00117
0.00308	0.00308
0.01015	0.01015

2dF

rξ(r) for samples with the following space density:

Old Galform	New Galform
0.00117	0.00117
0.00249	0.00249