M. Costanzi

Dark energy survey year 3 results: Cosmological constraints from cluster abundances, weak lensing, and galaxy clustering

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

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: Simulation-based cosmological inference with wavelet harmonics, scattering transforms, and moments of weak lensing mass maps. Validation on simulations

SPT clusters with DES and HST weak lensing. I. Cluster lensing and Bayesian population modeling of multiwavelength cluster datasets

Examining the self-interaction of dark matter through central cluster galaxy offsets

SPT-SZ MCMF: an extension of the SPT-SZ catalogue over the DES region

<i>Euclid</i> preparation

<i>Euclid</i> preparation

Euclid preparation. Sensitivity to neutrino parameters

<i>Euclid</i> preparation

Enhancing weak lensing redshift distribution characterization by optimizing the Dark Energy Survey Self-Organizing Map Photo-z method

Dark Energy Survey Year 3 results: Constraints on extensions to <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="normal">Λ</mml:mi><mml:mi>CDM</mml:mi></mml:math> with weak lensing and galaxy clustering

Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and <i>Planck</i>. III. Combined cosmological constraints

The Dark Energy Survey Year 3 and eBOSS: constraining galaxy intrinsic alignments across luminosity and colour space

<i>Euclid</i> preparation

Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mi>l</mml:mi><mml:mi>a</mml:mi><mml:mi>n</mml:mi><mml:mi>c</mml:mi><mml:mi>k</mml:mi></mml:mrow></mml:math>. II. Cross-correlation measurements and cosmological constraints

Timing the r-process Enrichment of the Ultra-faint Dwarf Galaxy Reticulum II

OzDES Reverberation Mapping Program: Hβ lags from the 6-yr survey

Characterizing the intracluster light over the redshift range 0.2 &amp;lt; <i>z</i> &amp;lt; 0.8 in the DES-ACT overlap

Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and<i>Planck</i>. I. Construction of CMB lensing maps and modeling choices

Measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel’dovich effect with SPT-3G and DES

Identification of Galaxy–Galaxy Strong Lens Candidates in the DECam Local Volume Exploration Survey Using Machine Learning

Mapping gas around massive galaxies: cross-correlation of DES Y3 galaxies and Compton-<i>y</i>maps from SPT and<i>Planck</i>

Cosmological shocks around galaxy clusters: a coherent investigation with DES, SPT, and ACT

Dark Energy Survey Year 3 results: redshift calibration of the <scp>MagLim</scp> lens sample from the combination of SOMPZ and clustering and its impact on cosmology

Euclid preparation. XXXIX. The effect of baryons on the Halo Mass Function

Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing