D. Gruen

This article explores Type Ia supernovae and their role in understanding the universe's expansion.

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.

DESI plays a crucial role in understanding galaxy redshifts and cosmic expansion.

Copacabana improves galaxy cluster membership identification and stellar mass estimation.

eROSITA's survey reveals extensive catalogs of X-ray sources across the sky.

Scientists study galaxy clusters to learn more about gravity and the universe's structure.

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.

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

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.

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

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

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