Sep 30 2019 By admin Minkowski Functionals and Minkowski Tensors in cosmology Simulating emission-line galaxies for ongoing and future BAO surveys When peaks, filaments or walls merge: forecasting special events through the coalescence of critical points Unveiling Cosmic Structure Formation by Cluster Lensing Intrinsic alignments of halo orientations with density and velocity fields at BAO scales and beyond Emulating Halo Statistics for Large-Scale Structure Cosmology ‹ Constraints on self-interacting dark matter from galaxy clusters up Minkowski Functionals and Minkowski Tensors in cosmology ›
