Constraining the halo bispectrum in real and redshift space from perturbation theory and non-linear stochastic bias
We present a method to produce mock galaxy catalogues with efficient perturbation theory schemes, which match the number density, power spectra and bispectra in real and in redshift space from N-body simulations. The essential contribution of this work is the way in which we constrain the bias parameters of the PATCHY-code. In addition to aiming at
Kitaura, F.-S. et al.
Fecha de publicación:
6
2015