to be central galaxies and thus not effected by tidal stripping at all.

The agreement with the observationally derived $w_p(r_p)$ for the catalogue including orphaned galaxies is very good, which is also reflected in the low value of $\chi_r^2(w_p) = 3.83$. Note that this value has been calculated with the parameters from the mass function fit given above and does not correspond to a fit to the projected CFs.

Note that we plot the projected CFs only up to $20\, {\rm
Mpc}$. Because of the finite box size, the clustering of host halos and thus central galaxies is underpredicted at large scales independent of mass. Additionally, due to the lack of long-wavelength modes, massive halos and galaxies can be underproduced leading to an underprediction of $w_p$ for the massive objects, independent of scale. However, the latter effect is very small, since the abundance of the massive halos in our simulation agrees very well with the predicted average [@sheth1999].

As a test we also used the present mass instead of the maximum mass for subhalos. We then found that the projected CF was underpredicted particularly on small scales. This effect is due to tidal stripping of subhalos and is thus strongest 