no code implementations • 1 Apr 2019 • Seshadri Nadathur, Paul M. Carter, Will J. Percival, Hans A. Winther, Julian Bautista
Combining void information with that from BAO and galaxy RSD in the same CMASS sample, we measure $D_A(0. 57)/r_s=9. 36\pm0. 07$ (at 0. 75% precision), $H(0. 57)r_s=(14. 03\pm0. 16)\;10^3$ kms$^{-1}$Mpc$^{-1}$ (1. 1%) and $f\sigma_8=0. 450\pm0. 019$ (4. 2%), consistent with cosmic microwave background (CMB) measurements from Planck.
Cosmology and Nongalactic Astrophysics
