We present cosmological results from the measurement of baryon acoustic oscillations
(BAO) in galaxy, quasar and Lyman-$\alpha $ forest tracers from the first year of …

We present the measurement of Baryon Acoustic Oscillations (BAO) from the Lyman-$\alpha
$(Ly $\alpha $) forest of high-redshift quasars with the first-year dataset of the Dark Energy …

We present the DESI 2024 galaxy and quasar baryon acoustic oscillations (BAO)
measurements using over 5.7 million unique galaxy and quasar redshifts in the range 0.1< …

We derive constraints on cosmological parameters and tests of dark energy models from the
combination of baryon acoustic oscillation (BAO) measurements with cosmic microwave …

We present angular diameter measurements obtained by measuring the position of baryon
acoustic oscillations (BAO) in an optimized sample of galaxies from the first three years of …

The goal of the Dark Energy Spectroscopic Instrument (DESI) is to determine the nature of
dark energy through the most precise measurement of the expansion history of the universe …

We present measurements of the Baryon Acoustic Oscillation (BAO) scale in redshift-space
using the clustering of quasars. We consider a sample of 147 000 quasars from the …

Baryon acoustic oscillations (BAO) involve measuring the spatial distribution of galaxies to
determine the growth rate of cosmic structures. We derive constraints on cosmological …

Low-redshift measurements of baryon acoustic oscillations (BAO) measure the late-time
evolution of the Universe and are a vital probe of dark energy. Over the past decade both the …

Baryon acoustic oscillations (BAOs) allow us to determine the expansion history of the
universe, thereby shedding light on the nature of dark energy. Recent observations of BAOs …