E. Gaztañaga

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

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

Extended dark energy analysis using DESI DR2 BAO 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

Comparing the DES-SN5YR and Pantheon+ SN cosmology analyses: investigation based on ‘evolving dark energy or supernovae systematics’?

Comparing Compressed and Full-Modeling analyses with FOLPS: implications for DESI 2024 and beyond

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

Production of alternate realizations of DESI fiber assignment for unbiased clustering measurement in data and simulations

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

Evidence for large baryonic feedback at low and intermediate redshifts from kinematic Sunyaev-Zel’dovich observations with ACT and DESI photometric galaxies

HOD-dependent systematics in Emission Line Galaxies for the DESI 2024 BAO analysis

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

Analytical and EZmock covariance validation for the DESI 2024 results

Validating the galaxy and quasar catalog-level blinding scheme for the DESI 2024 analysis

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

DESI peculiar velocity survey – Fundamental Plane

The Dark Energy Survey Supernova Program: an updated measurement of the Hubble constant using the inverse distance ladder

HOD-dependent systematics for luminous red galaxies in the DESI 2024 BAO analysis

Backlighting extended gas halos around luminous red galaxies: Kinematic Sunyaev-Zel’dovich effect from DESI Y1 and ACT data

Constraining the phase shift of relativistic species in DESI BAOs

Construction of the damped <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mi>Ly</mml:mi> <mml:mi>α</mml:mi> </mml:mrow> </mml:math> absorber catalog for DESI DR2 <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"> <mml:mrow> <mml:mrow> <mml:mrow> <mml:mi>Ly</mml:mi> <mml:mi>α</mml:mi> </mml:mrow> </mml:mrow> </mml:mrow> </mml:math> BAO

Dark Energy Survey Year 3 results: Simulation-based cosmological inference with wavelet harmonics, scattering transforms, and moments of weak lensing mass maps. II. cosmological results

Exploring the interaction between the MW and LMC with a large sample of blue horizontal branch stars from the DESI survey

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

Mitigating imaging systematics for DESI 2024 emission Line Galaxies and beyond