The association between gas and galaxies II : the two-point correlation function.

We measure the two-point correlation function, ξAG, between galaxies and quasar absorption-line systems at z 1017 cm2. For C iv absorbers, the peak strength of ξAG is roughly comparable to that of H i absorbers with NH I > 1016.5 cm2, consistent with the finding that the C iv absorbers are associated with strong H i absorbers. We do not reproduce the differences reported by Chen et al. between 1D ξAG measurements using galaxy subsamples of different spectral types. However, the full impact on the measurements of systematic differences in our samples is hard to quantify. We compare the observations with smoothed particle hydrodynamical (SPH) simulations and discover that in the observations ξAG is more concentrated to the smallest separations than in the simulations. The latter also display a 'finger of god' elongation of ξAG along the LOS in redshift space, which is absent from our data, but similar to that found by Ryan-Weber for the cross-correlation of quasar absorbers and H i-emission-selected galaxies. The physical origin of these 'fingers of god' is unclear, and we thus highlight several possible areas for further investigation