The Origins of [C II] Emission in Local Star-forming Galaxies
ASTROPHYSICAL JOURNAL 845:2 (2017) ARTN 96
Calibrating photometric redshifts with intensity mapping observations
PHYSICAL REVIEW D 96:4 (2017) ARTN 043515
Galaxy-halo alignments in the Horizon-AGN cosmological hydrodynamical simulation
Monthly Notices of the Royal Astronomical Society (2017)
Abstract:
Intrinsic alignments of galaxies are a significant astrophysical systematic affecting cosmological constraints from weak gravitational lensing. Obtaining numerical predictions from hydrodynamical simulations of expected survey volumes is expensive, and a cheaper alternative relies on populating large dark matter-only simulations with accurate models of alignments calibrated on smaller hydrodynamical runs. This requires connecting the shapes and orientations of galaxies to those of dark matter haloes and to the large-scale structure. In this paper, we characterise galaxy-halo alignments in the Horizon-AGN cosmological hydrodynamical simulation. We compare the shapes and orientations of galaxies in the redshift range $0Large sSynoptic Survey Telescope Galaxies Science Roadmap
(2017)