Baryon Acoustic Oscillations from the C IV Forest with DESI DR2

TL;DR

This paper reports the first detection of Baryon Acoustic Oscillations in the CIV forest using DESI DR2 data, providing precise measurements of cosmic distance scales at redshifts around 1.5 to 2.0.

Contribution

It introduces the first measurement of BAO in CIV absorption cross-correlated with quasars and ELGs, utilizing the extensive DESI DR2 dataset.

Findings

BAO detected at 4.2σ in CIV×QSO cross-correlation

Measured D_V/r_d at z=1.92 with 3.0% precision

First detection of BAO in CIV×ELG cross-correlation at 2.5σ

Abstract

We present a measurement of Baryon Acoustic Oscillations (BAO) in the cross-correlation of triply ionized carbon C IV absorption with the positions of quasars (QSO) and Emission Line Galaxies (ELG). We use quasars and ELGs from the second data release (DR2) of the Dark Energy Spectroscopic Instrument (DESI) survey. Our data sample consists of 2.5 million quasars, 3.1 million ELGs, and the C IV absorption is measured along the line of sight of 1.5 million high redshift quasars with $z > 1.3$. We measure the isotropic BAO signal at 4.2$\sigma$ for the CIV$\times$QSO cross-correlation. This translates into a 3.0% precision measurement of the ratio of the isotropic distance scale, $D_{\rm V}$, and the sound horizon at the drag epoch, $r_{\rm d}$, with $D_{\rm V}/r_{\rm d}(z_{\rm eff} = 1.92) = 30.3 \pm 0.9$. We make the first detection of the BAO feature in the CIV$\times$ELG cross-correlation at a significance of 2.5$\sigma$ and find $D_{\rm V}/r_{\rm d}(z_{\rm eff} = 1.47) = 24.6 \pm 1.0$.