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FLAMINGO
The FLAMINGO project
The FLAMINGO project
Determining satellite infall times using machine learning
Why are we still using 3D masses for cluster cosmology?
Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses
A high-resolution cosmological simulation of a strong gravitational lens
How baryons can significantly bias cluster count cosmology
Connecting the dots : analysis, development and applications of the SimpleX algorithm