Biased Tracers in Redshift Space in the EFT of Large-Scale Structure
  The Effective Field Theory of Large-Scale Structure (EFTofLSS) provides a
novel formalism that is able to accurately predict the clustering of
large-scale structure (LSS) in the mildly non-linear regime. Here we provide
the first computation of the power spectrum of biased tracers in redshift space
at one loop order, and we make the associated code publicly available. We
compare the multipoles $\ell=0,2$ of the redshift-space halo power spectrum,
together with the real-space matter and halo power spectra, with data from
numerical simulations at $z=0.67$. For the samples we compare to, which have a
number density of $\bar n=3.8 \cdot 10^{-2}(h \ {\rm Mpc}^{-1})^3$ and $\bar
n=3.9 \cdot 10^{-4}(h \ {\rm Mpc}^{-1})^3$, we find that the calculation at
one-loop order matches numerical measurements to within a few percent up to
$k\simeq 0.43 \ h \ {\rm Mpc}^{-1}$, a significant improvement with respect to
former techniques. By performing the so-called IR-resummation, we find that the
Baryon Acoustic Oscillation peak is accurately reproduced. Based on the results
presented here, long-wavelength statistics that are routinely observed in LSS
surveys can be finally computed in the EFTofLSS. This formalism thus is ready
to start to be compared directly to observational data.
