Density distribution of the cosmological matter field
The one-point probability distribution function (PDF) of the matter density field in the universe is a fundamental property that plays an essential role in...
Density weighted angular redshift fluctuations: a new cosmological observable
We propose the use of angular fluctuations in the galaxy redshift field as a new way to extract cosmological information in the Universe. This new probe $\delta...
DESI DR2 results. I. Baryon acoustic oscillations from the Lyman alpha forest
We present the baryon acoustic oscillation (BAO) measurements with the Lyman- α ( Ly α) forest from the second data release (DR2) of the Dark Energy...
DESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints
We present baryon acoustic oscillation (BAO) measurements from more than 14 million galaxies and quasars drawn from the Dark Energy Spectroscopic Instrument...
Detailed Theoretical Predictions for the Outskirts of Dark Matter Halos
In the present work we describe the formalism necessary to derive the properties of dark matter halos beyond 2 virial radii using the spherical collapse model...
Detection of Anomalous Microwave Emission in the Perseus Molecular Cloud with the COSMOSOMAS Experiment
We present direct evidence for anomalous microwave emission in the Perseus molecular cloud, which shows a clear rising spectrum from 11 to 17 GHz in the data...
Detection of the 2175 Å Extinction Feature at z = 0.83
We determine the extinction curve in the zl=0.83 lens galaxy of the gravitational lens SBS 0909+532 from the wavelength dependence of the flux ratio between the...
Detection of the Effect of Cosmological Large-Scale Structure on the Orientation of Galaxies
Galaxies are not distributed randomly throughout space but are instead arranged in an intricate ``cosmic web'' of filaments and walls surrounding bubble-like...