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(21 - 40 of 201)

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The PAU survey
Euclid
Euclid preparation
Euclid preparation. XV. Forecasting cosmological constraints for the Euclid and CMB joint analysis
Why are we still using 3D masses for cluster cosmology?
Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses
Forecasting the potential of weak lensing magnification to enhance LSST large-scale structure analyses
Euclid preparation
Extending empirical constraints on the SZ-mass scaling relation to higher redshifts via HST weak lensing measurements of nine clusters from the SPT-SZ survey at z >= 1
Euclid preparation
The dark matter halo masses of elliptical galaxies as a function of observationally robust quantities
Euclid
The PAU Survey
The PAU Survey
The HST See Change program
The mass-size relation of galaxy clusters
The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at 0 < z < 1.5
KiDS-1000: Constraints on the intrinsic alignment of luminous red galaxies
Mass calibration of distant SPT galaxy clusters through expanded weak-lensing follow-up observations with HST, VLT, & Gemini-South

Pages