A new analysis of galaxy 2-point functions in the BOSS survey, including
  full-shape information and post-reconstruction BAO
  We present a new method for consistent, joint analysis of the pre- and
post-reconstruction two-point functions of the BOSS survey. The
post-reconstruction correlation function is used to accurately measure the
distance-redshift relation and expansion history, while the pre-reconstruction
power spectrum multipoles constrain the broad-band shape and the rate-of-growth
of large-scale structure. Our technique uses Lagrangian perturbation theory to
self-consistently work at the level of two-point functions, i.e.\ directly with
the measured data, without approximating the constraints with summary
statistics normalized by the drag scale. Combining galaxies across the full
redshift range and both hemispheres we constrain $\Omega_m=0.303 \pm 0.0082$,
$H_0=69.23 \pm 0.77$ and $\sigma_8=0.733 \pm 0.047$ within the context of
$\Lambda$CDM. These constraints are in good agreement both with the Planck
primary CMB anisotropy data and recent cosmic shear surveys.
