The current standard model of cosmology successfully describes a variety of measurements,
but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid …

The current standard model of cosmology successfully describes a variety of measurements,
but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid …

Line-intensity mapping (LIM) is an emerging technique to probe the large-scale structure of
the Universe. By targeting the integrated intensity of specific spectral lines, it captures the …

The fiducial cosmological analyses of imaging surveys like DES typically probe the Universe
at redshifts z< 1. We present the selection and characterization of high-redshift galaxy …

The cosmic infrared background (CIB) is the accumulated infrared (IR) radiation mainly from
interstellar dust heated up by early stars. In this work, we measure the cross-correlation …

We present a Bayesian inference method to characterise the dust emission properties using
the well-known dust-correlation in the diffuse interstellar medium at Planck frequencies ν≥ …

We measure the cross-correlation between cosmic shear from the third-year release of the
Dark Energy Survey, thermal Sunyaev-Zel'dovich (tSZ) maps from Planck, and X-ray maps …

Cosmology is currently sitting on a ticking time bomb that will result in an unprecedented
explosion in the quantity and quality of data. In preparation, physicists are starting to …

The current standard model of cosmology successfully describes a variety of measurements,
but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid …

A century of ever improving observations has resulted in a concordance cosmological model
that is surprisingly simple: only six numbers are currently needed to describe a wide variety …