2014/04/30 by Matthew M. Pieri · 1 citation
Physics and Astronomy · #astro-ph.CO
paper · pdf · doi:10.1093/mnrasl/slu142
6 pages, 3 figures. Final version published in MNRAS Letters
arxiv created 2014/10/20 · arxiv updated 2015/06/19
In light of recent successes in measuring baryon acoustic oscillations in quasar absorption using the Lyman α (Lyα) transition, I explore the possibility of using the 1548Å transition of triply ionized carbon (C IV) as a tracer. While the Ly-alpha forest is a more sensitive tracer of intergalactic gas, it is limited by the fact that it can only be measured in the optical window at redshifts z > 2. Quasars are challenging to identify and observe at these high-redshifts, but the C IV forest can be probed down to redshifts z ≈ 1.3, taking full advantage of the peak in the redshift distribution of quasars that can be targeted with high efficiency. I explore the strength of the C IV absorption signal and show that the absorbing population on the red side of the Ly-alpha emission line is dominated by C IV (and so will dominate over the potential BAO signal of other metals). As a consequence, I argue that forthcoming surveys may have a sufficient increase in quasar number density to offset the lower sensitivity of the C IV forest and provide competitive precision using both the C IV autocorrelation and the C IV-quasar cross-correlation at < z > ≈ 1.6.