Gravitational Lensing in Clusters of Galaxies
arXiv:astro-ph/9905009 · doi:10.1143/PTPS.133.1
Abstract
Gravitational lensing in clusters of galaxies is an efficient tool to probe the mass distribution of galaxies and clusters, high redshift objects thanks to the gravitational amplification, and the geometry of the universe. We review some important aspects of cluster lensing and related issues in observational cosmology.
invited review of the journal: Progress of Theoretical Physics (in press) 51 pages - 33 figures
Cited by in corpus (26)
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- The Dark Matter Distribution in the Central Regions of Galaxy Clusters: Implications for CDM
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- Cluster Mass Profiles from a Bayesian Analysis of Weak Lensing Distortion and Magnification Measurements: Applications to Subaru Data
- Cluster-galaxy weak lensing
- Mass and Hot Baryons in Massive Galaxy Clusters from Subaru Weak Lensing and AMiBA SZE Observations
- A uniform X-ray analysis of 79 distant galaxy clusters with ROSAT and ASCA
- Numerical study of statistical properties of the lensing excursion angles
- Weak lensing Analysis of X-Ray-selected XXL Galaxy Groups and Clusters with Subaru HSC Data
- Chandra Analysis and Mass Estimation of the Lensing Cluster of Galaxies CL0024+17
- Suzaku Observations of the Centaurus Cluster: Absence of Bulk Motions in the Intracluster Medium
- Cooling flows or warming rays?
- Chandra Observations of SDSS J1004+4112: Constraints on the Lensing Cluster and Anomalous X-Ray Flux Ratios of the Quadruply Imaged Quasar
- Weak Lensing of Galaxy Clusters in MOND
- A possible route to spontaneous reduction of the heat conductivity by a temperature gradient driven instability in electron-ion plasmas
- Halo model prediction of the cosmic magnification statistics: the full non-linear contribution
- Suzaku Observations of Iron K-lines from the Intracluster Medium of the Coma Cluster
- Bounds on graviton mass using weak lensing and SZ effect in galaxy clusters
- X-ray Spectroscopy of Clusters of Galaxies
- The SOAR Gravitational Arc Survey - I: Survey overview and photometric catalogs
- Gravitational Lensing by Nearby Clusters of Galaxies
- Discovery of a Strongly Lensed Galaxy at z=3.9 behind a z=0.83 Galaxy Cluster
- relensing: Reconstructing the mass profile of galaxy clusters from gravitational lensing
- The KALEIDOSCOPE survey : A new strong and weak gravitational lensing view of the massive galaxy cluster MACS J1423.8+2404
- The Kaleidoscope Survey: Strong Gravitational Lensing in Galaxy Clusters with Radial Arcs