The intrinsic alignment of galaxies and its impact on weak gravitational lensing in an era of precision cosmology
From MaRDI portal
Publication:516863
DOI10.1016/j.physrep.2014.11.001zbMath1357.85002arXiv1407.6990OpenAlexW3102350624MaRDI QIDQ516863
Publication date: 15 March 2017
Published in: Physics Reports (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1407.6990
Galactic and stellar structure (85A15) Astrophysical cosmology (85A40) Statistical astronomy (85A35)
Related Items (12)
Lagrangian approach to super-sample effects on biased tracers at field level: galaxy density fields and intrinsic alignments ⋮ Efficient optimal reconstruction of linear fields and band-powers from cosmological data ⋮ An EFT description of galaxy intrinsic alignments ⋮ Beyond Limber: efficient computation of angular power spectra for galaxy clustering and weak lensing ⋮ Primordial gravitational waves from galaxy intrinsic alignments ⋮ Field-level inference of galaxy intrinsic alignment from the SDSS-III BOSS survey ⋮ Parity violation in weak interactions: how experiment can shape a theoretical framework ⋮ Environmental dependence of ellipticity correlation functions of intrinsic alignments ⋮ Direct probe of dark energy through gravitational lensing effect ⋮ Intrinsic galaxy alignment from angular dependent primordial non-Gaussianity ⋮ FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory ⋮ Galaxy imaging surveys as spin-sensitive detector for cosmological colliders
Uses Software
Cites Work
- Unnamed Item
- Halo models of large scale structure
- Cosmological tests of gravity
- Weak gravitational lensing
- Large-scale structure of the universe and cosmological perturbation theory
- Weak lensing, dark matter and dark energy
- Remarks on the formulation of the cosmological constant/dark energy problems
- Gravitational lensing
- The removal of shear-ellipticity correlations from the cosmic shear signal via nulling techniques
- Gravitational lensing: a unique probe of dark matter and dark energy
- GALACTIC ANGULAR MOMENTA AND ANGULAR MOMENTUM CORRELATIONS IN THE COSMOLOGICAL LARGE-SCALE STRUCTURE
- Light propagation in arbitrary spacetimes and the gravitational lens approximation
- Cosmological weak lensing
- Intrinsic alignment boosting
- The removal of shear-ellipticity correlations from the cosmic shear signal
This page was built for publication: The intrinsic alignment of galaxies and its impact on weak gravitational lensing in an era of precision cosmology