Large-scale environment of z~5.7 CIV absorption systems I: projected distribution of galaxies

TL;DR

This study investigates the environments of CIV absorption systems at redshift 5.7, finding they are associated with low-mass galaxies like LAEs rather than massive LBGs, suggesting faint galaxies dominate ionization at this epoch.

Contribution

It provides the first detailed analysis of the galaxy environments of high-redshift CIV systems, highlighting the role of low-mass galaxies in early universe ionization.

Findings

CIV systems are located >10h$^{-1}$ Mpc from LBG concentrations.

An excess of LAEs is found near CIV systems, indicating their potential as sources.

Strong CIV absorption at z~5.7 traces low-density environments dominated by low-mass galaxies.

Abstract

Metal absorption systems are products of star formation. They are believed to be associated with massive star forming galaxies, which have significantly enriched their surroundings. To test this idea with high column density CIV absorption systems at z~5.7, we study the projected distribution of galaxies and characterise the environment of CIV systems in two independent quasar lines-of-sight: J103027.01+052455.0 and J113717.73+354956.9. Using wide field photometry (~80x60h$^{-1}$ comoving Mpc), we select bright (Muv(1350\AA)<-21.0 mag.) Lyman break galaxies (LBGs) at z~5.7 in a redshift slice \Delta z~0.2 and we compare their projected distribution with z~5.7 narrow-band selected Lyman alpha emitters (LAEs, \Delta z~0.08). We find that the CIV systems are located more than 10h$^{-1}$ projected comoving Mpc from the main concentrations of LBGs and no candidate is closer than ~5h$^{-1}$ projected comoving Mpc. In contrast, an excess of LAEs -lower mass galaxies- is found on scales of ~10h$^{-1}$ comoving Mpc, suggesting that LAEs are the primary candidates for the source of the CIV systems. Furthermore, the closest object to the system in the field J1030+0524 is a faint LAE at a projected distance of 212h$^{-1}$ physical kpc. However, this work cannot rule out undiscovered lower mass galaxies as the origin of these absorption systems. We conclude that, in contrast with lower redshift examples (z<3.5), strong CIV absorption systems at z~5.7 trace low-to-intermediate density environments dominated by low-mass galaxies. Moreover, the excess of LAEs associated with high levels of ionizing flux agrees with the idea that faint galaxies dominate the ionizing photon budget at this redshift.