Dragan Huterer

Dark Energy Survey: Implications for cosmological expansion models from the final DES baryon acoustic oscillation and supernova data

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

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

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

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

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

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

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

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

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

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

Dark Energy Survey Year 6 Results: Synthetic-source Injection Across the Full Survey Using Balrog

Dark Energy Survey Year 6 Results: Cell-based Coadds and Metadetection Weak Lensing Shape Catalogue

Dark Energy Survey: Implications for cosmological expansion models from the final DES baryon acoustic oscillation and supernova data

SPT clusters with DES and HST weak lensing. II. Cosmological constraints from the abundance of massive halos

Weak lensing combined with the kinetic Sunyaev–Zel’dovich effect: a study of baryonic feedback

Dark Energy Survey: A 2.1% measurement of the angular baryonic acoustic oscillation scale at redshift <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>z</mml:mi></mml:mrow><mml:mrow><mml:mi>eff</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn>0.85</mml:mn></mml:mrow></mml:math> from the final dataset

Dark energy survey year 3 results: likelihood-free, simulation-based <i>w</i>CDM inference with neural compression of weak-lensing map statistics

Cosmological constraints from the tomography of DES-Y3 galaxies with CMB lensing from ACT DR4

Dark energy survey year 3 results: cosmology from galaxy clustering and galaxy–galaxy lensing in harmonic space

Cosmology from cross-correlation of ACT-DR4 CMB lensing and DES-Y3 cosmic shear

Towards Robust Measurements of H0 with Dark Standard Candles

Collaborative Research: New Avenues to Cosmic Acceleration

Graduate Student Support for COSMO-16 International Cosmology Conference

Probing the Primordial Universe with the Large-Scale Structure and the CMB: from Systematic Errors to Fundamental Physics

Testing the Statistical Isotropy of the Universe

Towards Understanding of Properties and Nature of Dark Energy