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Works cited by this work

COSMOLOGICAL CONSTRAINTS FROM SUNYAEV–ZEL'DOVICH-SELECTED CLUSTERS WITH X-RAY OBSERVATIONS IN THE FIRST 178 deg<sup>2</sup> OF THE SOUTH POLE TELESCOPE SURVEY

Practical Weak-lensing Shear Measurement with Metacalibration

First results from the IllustrisTNG simulations: the galaxy colour bimodality

First results from the IllustrisTNG simulations: a tale of two elements – chemical evolution of magnesium and europium

First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Dark Energy Survey year 1 results: Cosmological constraints from galaxy clustering and weak lensing

The Galaxy Cluster Mass Scale and Its Impact on Cosmological Constraints from the Cluster Population

Constraints on Cosmological Parameters from the 500 deg<sup>2</sup> SPTPOL Lensing Power Spectrum

Cluster–galaxy weak lensing

Dark Energy Survey Year 3 Results: Photometric Data Set for Cosmology

Untitled

Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing

The eROSITA Final Equatorial-Depth Survey (eFEDS)

Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing

<scp>nautilus</scp>: boosting Bayesian importance nested sampling with deep learning

Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations

New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant

Untitled

Understanding parameter differences between analyses employing nested data subsets

Untitled

An improved SPH scheme for cosmological simulations

CONNECTING ANGULAR MOMENTUM AND GALACTIC DYNAMICS: THE COMPLEX INTERPLAY BETWEEN SPIN, MASS, AND MORPHOLOGY

ON THE ACCURACY OF WEAK-LENSING CLUSTER MASS RECONSTRUCTIONS

Constraints on Cosmological Parameters from Future Galaxy Cluster Surveys

MASS CALIBRATION AND COSMOLOGICAL ANALYSIS OF THE SPT-SZ GALAXY CLUSTER SAMPLE USING VELOCITY DISPERSION σ<sub><i>v</i></sub>AND X-RAY<i>Y</i><sub>X</sub>MEASUREMENTS