Probing Large-scale UV Background Inhomogeneity Associated with Quasars using Metal Absorption

TL;DR

This study investigates large-scale UV background inhomogeneity linked to quasars at high redshift by analyzing metal absorption in quasar spectra, revealing significant inhomogeneities on tens of megaparsecs.

Contribution

It demonstrates the measurement of UV background inhomogeneity on large scales using metal absorption, highlighting the impact of quasars on the intergalactic medium.

Findings

Stronger high ionization species absorption closer to quasars

O VI absorption shows the most significant change

Metal absorption sensitivity to quasar proximity is confirmed

Abstract

We study large-scale UV background inhomogeneity in three-dimensions associated with the observed quasar populations at high redshift. We do this by measuring metal absorption through quasar absorption spectrum stacking as a function distance to closest quasar in SDSS-IV/eBOSS on 10s of comoving megaparsec scales. We study both intergalactic medium absorbers and mixed circumgalactic medium absorbers and probe absorption in O VI, C IV, and Si IV, and Si III. Overall stronger high ionization species absorption is seen closer to quasars at $2.4<z<3.1$. O VI absorption shows a particularly strong change, with effects in C IV evident in some cases, and more marginal effects in Si III and Si IV. We further study $2.05<z<2.4$ (with weak signs of increasing homogeneity with time) and explore the study of metal absorption as a function of integrated SDSS-r band flux quasar flux (yielding consistent but less significant results). While the metal absorption does show sensitivity to large-scale 3D quasar proximity, the current incomplete quasar samples limit detailed interpretation. This work does, however, demonstrate that UV background inhomogeneities exist on scales of several 10s of comoving megaparsecs associated with quasars and that they can be measured with precision by examining metal absorption in the intergalactic medium.