D. Kirkby

DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations

DESI DR2 results. II. Measurements of baryon acoustic oscillations and cosmological constraints

DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman alpha forest

DESI 2024 III: baryon acoustic oscillations from galaxies and quasars

DESI 2024 VII: cosmological constraints from the full-shape modeling of clustering measurements

DESI 2024 II: sample definitions, characteristics, and two-point clustering statistics

DESI 2024 V: Full-Shape galaxy clustering from galaxies and quasars

Constraints on neutrino physics from DESI DR2 BAO and DR1 full shape

Dynamical dark energy in light of the DESI DR2 baryonic acoustic oscillations measurements

Modified gravity constraints from the full shape modeling of clustering measurements from DESI 2024

Constraining primordial non-Gaussianity with DESI 2024 LRG and QSO samples

Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Validation of the DESI DR2 measurements of baryon acoustic oscillations from galaxies and quasars

Fiducial-cosmology-dependent systematics for the DESI 2024 BAO analysis

Characterization of DESI fiber assignment incompleteness effect on 2-point clustering and mitigation methods for DR1 analysis

Measuring σ ₈ using DESI Legacy Imaging Surveys Emission-Line galaxies and Planck CMB lensing, and the impact of dust on parameter inference

Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data

A sound horizon-free measurement of <i>H</i> ₀ in DESI 2024

Positive Neutrino Masses with DESI DR2 via Matter Conversion to Dark Energy

Characterization of contaminants in the Lyman-alpha forest auto-correlation with DESI

Stellar reddening map from DESI imaging and spectroscopy

DESI DR1 Lyα 1D power spectrum: the optimal estimator measurement

Model-independent measurement of the matter-radiation equality scale in DESI 2024

Overview of the Fiber System for the Dark Energy Spectroscopic Instrument

Analysis of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>DESI</mml:mi><mml:mo stretchy="false">×</mml:mo><mml:mi>DES</mml:mi></mml:mrow></mml:math> using the Lagrangian effective theory of LSS

The Atacama Cosmology Telescope DR6 and DESI: structure formation over cosmic time with a measurement of the cross-correlation of CMB lensing and luminous red galaxies

Archetype-based Redshift Estimation for the Dark Energy Spectroscopic Instrument Survey

Broad absorption line quasars in the Dark Energy Spectroscopic Instrument Early Data Release

The Spectroscopic Data Processing Pipeline for the Dark Energy Spectroscopic Instrument

Survey Operations for the Dark Energy Spectroscopic Instrument