BOSS full-shape analysis from the EFTofLSS with exact time dependence
  We re-analyze the full shape of BOSS galaxy two-point function from the
Effective-Field Theory of Large-Scale Structure at the one loop within
$\Lambda$CDM with massive neutrinos using a big bang nucleosynthesis (BBN)
prior, removing the Einstein-de Sitter (EdS) approximation in the time
dependence of the loop, and, properly accounting for the redshift selection
over the BOSS samples instead of assuming an effective redshift. We constrain,
at $68\%$-confidence level (CL), the present-day matter fraction to
$\Omega_m=0.322 \pm 0.018$, the Hubble constant to $H_0=69.1\pm 0.14$
(km/s)/Mpc, the $\log$-amplitude of the primordial spectrum to $\ln (10^{10}
A_s) = 2.97 \pm 0.25$, the spectral tilt to $n_s = 0.938 \pm 0.082$, and bound
the total neutrino mass to $<1.1$ at $95\%$-CL. We find no significant shift in
the posteriors of the cosmological parameters due to the EdS approximation, but
a marginal difference in $\ln (10^{10} A_s)$ due to the effective redshift
approximation of about $0.4\sigma$, where $\sigma$ is the $68\%$-confidence
interval. Regarding the EdS approximation, we check that the same conclusion
holds on simulations of volume like DESI in $\Lambda$CDM and $w$CDM, with a BBN
prior. In contrast, for an approximate, effective redshift, to be assumed, we
advocate systematic assessments on redshift selection for ongoing and future
large-volume surveys.
