A. Carnero Rosell

This study investigates the relationship between intra-cluster light and galaxy cluster mass.

Study reveals important connections between CMB and galaxy weak lensing.

A software package for studying galaxy clusters and their properties using cosmic survey data.

Copacabana improves galaxy cluster membership identification and stellar mass estimation.

New techniques enhance identification of Type Ia supernovae, aiding cosmological studies.

DESI enhances galaxy observations, improving our grasp of cosmic structures.

DESI's data sheds light on dark energy and cosmic expansion.

This study analyzes Baryon Acoustic Oscillations using data from the Dark Energy Spectroscopic Instrument.

The DESI project enhances measurements of Baryon Acoustic Oscillations in the universe.

Investigating baryonic feedback impacts on weak lensing and cosmological parameters.

Reverberation mapping aids scientists in studying black holes across the universe.

Learn how DESI creates catalogs of large-scale structures in the universe.

This study examines how weak lensing alters the brightness of supernovae.

Study examines how cosmological choices affect BAO measurements and insights into dark energy.

A look at how the Dark Energy Survey sheds light on cosmic mysteries.

Photometric redshifts offer a new method for studying Type Ia supernovae.

This study reveals new findings about faint galaxies and their role in the universe.

Study reveals how host galaxies affect Type Ia supernova brightness.

A study on how BCGs influence intracluster light and galaxy cluster evolution.

Researching galaxy clusters reveals insights into dark energy and modified gravity.

Astronomers tackle issues of galaxy observation using DESI's fiber assignment techniques.

DESI helps unveil the mysteries of dark energy and cosmic structures.

Discover how cosmic sound waves reveal the universe's growth and expansion.