We present a review of the current state of the art of cosmological dark matter simulations,
with particular emphasis on the implications for dark matter detection efforts and studies of …

An array of large observational programs using ground-based and space-borne telescopes
is planned in the next decade. The forthcoming wide-field sky surveys are expected to …

Based on a suite of state-of-the-art high-resolution N-body simulations, we revisit the so-
called halofit model as an accurate fitting formula for the nonlinear matter power spectrum …

Building on the legacy of the Sloan Digital Sky Survey (SDSS-I and II), SDSS-III is a program
of four spectroscopic surveys on three scientific themes: dark energy and cosmological …

We present Fisher matrix projections for future cosmological parameter measurements,
including neutrino masses, Dark Energy, curvature, modified gravity, the inflationary …

We present an improved prescription for the matter power spectrum in redshift space taking
proper account of both nonlinear gravitational clustering and redshift distortion, which are of …

We provide a simple, unified approach to describing the impact of super-sample covariance,
or beat coupling, on power spectrum estimation in a finite-volume survey. For a wide range …

We present a new N-body simulation from the Marenostrum Institut de Ciències de l'Espai
(MICE) collaboration, the MICE Grand Challenge (MICE-GC), containing about 70 billion …

We investigate how much can be learnt about four types of primordial non-Gaussianity
(PNG) from small-scale measurements of the halo field. Using the quijote-png simulations …

Using separate universe simulations, we accurately quantify super-sample covariance
(SSC), the typically dominant sampling error for matter power spectrum estimators in a finite …