We reproduce the galaxy clustering catalogue from the SDSS-III Baryon Oscillation
Spectroscopic Survey Final Data Release (BOSS DR11&DR12) with high fidelity on all …

Galactic archaeology based on star counts is instrumental to reconstruct the past mass
assembly of Local Group galaxies. The development of new observing techniques and data …

We produce 1000 realizations of synthetic clustering catalogues for each type of the tracers
used for the baryon acoustic oscillation and redshift space distortion analysis of the Sloan …

Accurate analyses of present and next-generation cosmological galaxy surveys require new
ways to handle effects of non-linear gravitational structure formation processes in data. To …

The Euclid mission–with its spectroscopic galaxy survey covering a sky area over 15 000
deg 2 in the redshift range 0.9< z< 1.8–will provide a sample of tens of thousands of cosmic …

Gravitational wave (GW) sources are an excellent probe of the luminosity distance and offer
a novel measure of the Hubble constant, H 0. This estimation of H 0 from standard sirens …

We derive cosmological constraints from the probability distribution function (PDF) of
evolved large-scale matter density fluctuations. We do this by splitting lines of sight by …

We present vide, the Void IDentification and Examination toolkit, an open-source
Python/C++ code for finding cosmic voids in galaxy redshift surveys and N-body simulations …

Detecting and measuring a non-Gaussian signature of primordial origin in the density field is
a major science goal of next-generation galaxy surveys. The signal will permit us to …

Cosmology inference of galaxy clustering at the field level with the EFT likelihood in
principle allows for extracting all non-Gaussian information from quasi-linear scales, while …