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= Gravitational lensing: weak
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Gravitational lensing: weak
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KiDS-1000: combined halo-model cosmology constraints from galaxy abundance, galaxy clustering, and galaxy-galaxy lensing
KiDS-1000: cross-correlation with Planck cosmic microwave background lensing and intrinsic alignment removal with self-calibration
KiDS-1000 cosmology: Constraints from density split statistics
KiDS-Legacy calibration: Unifying shear and redshift calibration with the SKiLLS multi-band image simulations
KiDS-1000: Cosmology with improved cosmic shear measurements
Dynamical cluster masses from photometric surveys
Consistent lensing and clustering in a low-S_8 Universe with BOSS, DES Year 3, HSC Year 1, and KiDS-1000
Euclid preparation
Euclid: covariance of weak lensing pseudo-Cl estimates
Pure-mode correlation functions for cosmic shear and application to KiDS-1000
KiDS and Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
Why are we still using 3D masses for cluster cosmology?
Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses
Mass calibration of distant SPT galaxy clusters through expanded weak-lensing follow-up observations with HST, VLT, & Gemini-South
Mitigating the effects of undersampling in weak lensing shear estimation with metacalibration
Accounting for object detection bias in weak gravitational lensing studies
A fully data-driven algorithm for accurate shear estimation
Euclid: Impact of non-linear and baryonic feedback prescriptions on cosmological parameter estimation from weak lensing cosmic shear
How baryons can significantly bias cluster count cosmology
The alignment of galaxies across all scales
