The detection of the accelerated expansion of the Universe has been one of the major
breakthroughs in modern cosmology. Several cosmological probes (Cosmic Microwave …

Shortly after its discovery, General Relativity (GR) was applied to predict the behavior of our
Universe on the largest scales, and later became the foundation of modern cosmology. Its …

We present GIGANTES, the most extensive and realistic void catalog suite ever released—
containing over 1 billion cosmic voids covering a volume larger than the observable …

Marked power spectra are two-point statistics of a marked field obtained by weighting each
location with a function that depends on the local density around that point. We consider …

The studies of disordered heterogeneous media and galaxy cosmology share a common
goal: analyzing the disordered distribution of particles and/or building blocks at microscales …

Abstract We develop a Lagrangian Perturbation Theory (LPT) framework to study the
clustering of cold dark matter (CDM) in cosmologies with massive neutrinos. We follow the …

We compute 1-loop corrections to the redshift space galaxy power spectrum in cosmologies
containing additional scales, and hence kernels different from Einstein-de Sitter (EdS) …

We perform a multi-tracer full-shape analysis in Fourier space based on the effective field
theory of large-scale structure (EFTofLSS) using the complete Sloan Digital Sky Survey IV …

Future large-scale structure surveys will measure the locations and shapes of billions of
galaxies. The precision of such catalogues will require meticulous treatment of systematic …

It is well known that the power spectrum is not able to fully characterize the statistical
properties of non-Gaussian density fields. Recently, many different statistics have been …