Studies of the geometry and energy content of the Universe, physics of cosmic expansion,
fundamental properties of standard model particles, and growth of structure remain the key …

This paper presents the PNG-UNITSIMS suite, which includes the largest full N-body
simulation to date with local primordial non-Gaussianities (local PNG), the PNG-UNIT. The …

Numerical simulations in cosmology require trade-offs between volume, resolution and run-
time that limit the volume of the Universe that can be simulated, leading to sample variance …

Modern redshift surveys are tasked with mapping out the galaxy distribution over enormous
distance scales. Existing hydrodynamical simulations, however, do not reach the volumes …

Context. We present a novel approach to the construction of mock galaxy catalogues for
large-scale structure analysis based on the distribution of dark matter halos obtained with …

In order to address fundamental questions related to the expansion history of the Universe
and its primordial nature with the next generation of galaxy experiments, we need to model …

Simulations have become an indispensable tool for accurate modelling of observables
measured in galaxy surveys, but can be expensive if very large dynamic range in scale is …

We investigate the nature of correlations in the small-scale flux statistics of the Lyman-α
(Lyα) forest across redshift bins. Understanding and characterising these correlations is …

The Dark Energy Spectroscopic Instrument (DESI) will provide unprecedented information
about the large-scale structure of our Universe. In this work, we study the robustness of the …

Observations of the Lyman-α forest in distant quasar spectra with upcoming surveys are
expected to provide significantly larger and higher-quality datasets. To interpret these …