Showing 41–60 of 206 results
/ Date/ Name
Dec 29, 2023Measuring the conditional luminosity and stellar mass functions of galaxies by combining the DESI LS DR9, SV3 and Y1 dataAug 11, 2017HBT+: an improved code for finding subhalos and building merger trees in cosmological simulationsAug 15, 2025Frequentist Cosmological Constraints from Full-Shape Clustering Measurements in DESI DR1Apr 16, 2025The "Little Dark Dot": Evidence for Self-interacting Dark Matter in the Strong Lens SDSS J0946+1006?May 13, 2025Modelling the impact of quasar redshift errors on the full-shape analysis of correlations in the Lyman-$α$ forestJan 27, 2025Measuring the Stellar-to-Halo Mass Relation at $\sim10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lensesOct 31, 2025Reproducing Abell 2744 with the HyperMillennium SimulationMar 3, 2025PAC in DESI. I. Galaxy Stellar Mass Function into the $10^{6}{\rm M}_{\odot}$ FrontierOct 25, 2020A forward-modelling method to infer the dark matter particle mass from strong gravitational lensesJul 29, 2021Baryon-driven decontraction in Milky Way mass haloesJan 8, 2021A sparse regression approach to modeling the relation between galaxy stellar masses and their host halosSep 13, 2012Dark Matter Halo Merger Histories Beyond Cold Dark Matter: I - Methods and Application to Warm Dark MatterJan 11, 2016The Mass-Concentration-Redshift Relation of Cold and Warm Dark Matter HalosDec 21, 2015Constraints on the identity of the dark matter from strong gravitational lensesNov 30, 2015Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical modelsJul 19, 2017The core-cusp problem: a matter of perspectiveNov 10, 2016Comparing semi-analytic particle tagging and hydrodynamical simulations of the Milky Way's stellar haloNov 10, 2009Physical constraints on the central mass and baryon content of satellite galaxiesApr 2, 2024The onset of bar formation in a massive galaxy at $z \sim 3.8$Dec 7, 2001The 2dF Galaxy Redshift Survey: The amplitudes of fluctuations in the 2dFGRS and the CMB, and implications for galaxy biasing