Dark sector, constituting about 95% of the Universe, remains the subject of numerous
studies. There are lots of models dealing with the cause of the effects assigned to “dark …

In the past 50 years, cosmology has gone from a field known for the errors being in the
exponents to a precision science. The transformation—powered by ideas, technology, a …

We present cosmological constraints from a gravitational lensing mass map covering 9400
deg 2 reconstructed from measurements of the cosmic microwave background (CMB) made …

We present the first cosmology results from large-scale structure using the full 5000 deg 2 of
imaging data from the Dark Energy Survey (DES) Data Release 1. We perform an analysis …

We present cosmological constraints from the analysis of angular power spectra of cosmic
shear maps based on data from the first three years of observations by the Dark Energy …

We constrain the matter density Ωm and the amplitude of density fluctuations σ8 within the
ΛCDM cosmological model with shear peak statistics and angular convergence power …

In this work, we present the galaxy clustering measurements of the two DES lens galaxy
samples: a magnitude-limited sample optimized for the measurement of cosmological …

We present a cosmological analysis using the second and third moments of the weak
lensing mass (convergence) maps from the first three years of data (Y3) data of the Dark …

We present simulation-based cosmological w CDM inference using Dark Energy Survey
Year 3 weak-lensing maps, via neural data compression of weak-lensing map summary …

We measure the impact of source galaxy clustering on higher order summary statistics of
weak gravitational lensing data. By comparing simulated data with galaxies that either trace …