SIMBAD references

We present a pilot study of the clustering properties of Lyα absorbers with respect to known galaxies based on 112 Lyα absorbers and 482 galaxies identified at z<0.5 along the sight line toward PKS 0405-123. The principal goal is to determine the origin of Lyα absorbers based on their cross-correlation amplitude with known galaxies and to investigate a possible N(H I) dependence of the cross-correlation function. The main results of our study are as follows: (1) The cross-correlation function ξ_ga measured using only emission-line-dominated galaxies and Lyα absorbers with logN(H I)≥14 shows a comparable strength to the galaxy autocorrelation function ξ_gg on comoving, projected distance scales of less than 1 h^–1 Mpc, while there remains a lack of cross-correlation signal when using only absorption-line-dominated galaxies. This signifies a morphology-dependent ξ_ga and indicates that strong absorbers with logN(H I)≥14 and emission-line galaxies reside in the same halo population. (2) A maximum likelihood analysis shows that Lyα absorbers with logN(H I)<13.6 are consistent with being more randomly distributed with respect to known galaxies. (3) Finally, we find based on this single sight line that the amplitude of ξ_ga does not depend sensitively on N(H I) for strong absorbers, with logN(H I)≥13.6.