BAO from the CIV Forest with DESI

We present a measurement of Baryon Acoustic Oscillations (BAO) in the cross-correlation of triply ionized carbon (CIV) 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 the Dark Energy Spectroscopic Instrument (DESI) survey. Our data sample consists of 2.5 million quasars, 3.1 million ELGs, and the CIV absorption is measured along the line of sight of 1.5 million high redshift quasars. We measure the isotropic BAO signal at 4.2σ for the CIV-QSO cross-correlation. This translates into a 3.0% precision measurement of the ratio of the isotropic distance scale, D_V, and the sound horizon at the drag epoch, r_d. We make the first detection of the BAO peak in the CIV-ELG cross-correlation at a significance of 2.5σ.