Cluster-galaxy weak lensing
arXiv:2007.00506 · doi:10.1007/s00159-020-00129-w
Abstract
Weak gravitational lensing of background galaxies provides a direct probe of the projected matter distribution in and around galaxy clusters. Here we present a self-contained pedagogical review of cluster--galaxy weak lensing, covering a range of topics relevant to its cosmological and astrophysical applications. We begin by reviewing the theoretical foundations of gravitational lensing from first principles, with special attention to the basics and advanced techniques of weak gravitational lensing. We summarize and discuss key findings from recent cluster--galaxy weak-lensing studies on both observational and theoretical grounds, with a focus on cluster mass profiles, the concentration--mass relation, the splashback radius, and implications from extensive mass calibration efforts for cluster cosmology.
arXiv commentInvited review article published in The Astronomy and Astrophysics Review (see https://rdcu.be/caSUp); a version that corrects references and errors introduced by the publisher during the production process; 102 pages, 30 figures
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- Mass accretion rates of the HectoMAP clusters of galaxies
- Cluster profiles from beyond-the-QE CMB lensing mass maps
- Weak-lensing tunnel voids in simulated light cones: A new pipeline to investigate modified gravity and massive neutrinos signatures
- Mass Modeling and Kinematics of Galaxy Clusters in Modified Gravity
- Testing the Collisionless Nature of Dark Matter with the Radial Acceleration Relation in Galaxy Clusters
- relensing: Reconstructing the mass profile of galaxy clusters from gravitational lensing
- Cosmic accretion shocks as a tool to measure the dark matter mass of galaxy clusters
- AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing
- CHEX-MATE: Multi-probe analysis of Abell 1689
- Radio emission from a massive node of the cosmic web. A discovery powered by machine learning
- Caustic and hydrostatic mass bias: Implications for modified gravity
- Constraining dark matter halo profiles with symbolic regression
- Gravitational lensing by an ellipsoidal Navarro--Frenk--White dark-matter halo: An analytic solution and its properties
- Peaks in weak lensing mass maps for cluster astrophysics and cosmology
- An empirical method for mitigating an excess up-scattering mass bias on the weak lensing mass estimates for shear-selected cluster samples
- Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters
- Kinematic Lensing Inference II: Cluster Lensing with (1) Galaxies
- Searching for rotation in X-COP galaxy clusters
- Galaxy cluster count cosmology with simulation-based inference
- Galaxy Cluster Mass Estimation Through The Splashback Radius
- The Three Hundred Project: dissecting the fundamental plane of galaxy clusters up to
- Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
- X-ray flux -- mass relation for galaxy clusters
- AMICO-WL: an optimal filtering algorithm for galaxy cluster detections with weak lensing
- HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters
- Comparison of HMG and flat rotation velocities inferred from galaxy-galaxy weak lensing
- Multi-scale weak lensing detection of galaxy clusters with source redshift tomography
- The Splashback Mass Function of Galaxy Clusters from Photometric Data
- Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
- CLASH-VLT: The Fifth Force in Chameleon Gravity from Joint Lensing and Kinematics Cluster Mass Profiles
- Gravitational Lensing By a Massive Object in a Dark Matter Halo. I. Critical Curves and Caustics
- The signature of major mergers on the hydrostatic mass bias of galaxy clusters
- Self-similarity of the mass distribution in rich galaxy clusters up z~1 tracked with weak lensing
- Galaxies in the central regions of simulated galaxy clusters
- The thermodynamic structure and large-scale structure filament in MACS J0717.5+3745
- Shear Mapping in Python (SMPy): Modular, Extensible, and Accessible Dark Matter Mapping
- A Spectroscopic View of the JWST/GTO Strong Lensing Cluster A1489
- Measuring weak lensing masses on individual clusters
- A novel inversion algorithm for weak gravitational lensing using quasi-conformal geometry
- Local environmental dependence on weak-lensing shear statistics
- A short review on joint weak and strong cluster lens-mass reconstruction