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We present a new method for consistent, joint analysis of the pre- andpost-reconstruction two-point functions of the BOSS survey. Thepost-reconstruction correlation function is used to accurately measure thedistance-redshift relation and expansion history, while the pre-reconstructionpower spectrum multipoles constrain the broad-band shape and the rate-of-growthof large-scale structure. Our technique uses Lagrangian perturbation theory toself-consistently work at the level of two-point functions, i.e.\ directly withthe measured data, without approximating the constraints with summarystatistics normalized by the drag scale. Combining galaxies across the fullredshift 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 Planckprimary CMB anisotropy data and recent cosmic shear surveys.

A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO