The C IV forest as a probe of baryon acoustic oscillations
  In light of recent successes in measuring baryon acoustic oscillations in
quasar absorption using the Lyman $\alpha$ (Ly$\alpha$) transition, I explore
the possibility of using the 1548\AA\ 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 $z \approx 1.3$, 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 $< z > \approx 1.6$.
