Calibrating photometric redshifts with intensity mapping observations
PHYSICAL REVIEW D 96:4 (2017) ARTN 043515
hi_class: Horndeski in the Cosmic Linear Anisotropy Solving System
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS (2017) ARTN 019
The Python Sky Model: software for simulating the Galactic microwave sky
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 469:3 (2017) 2821-2833
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)