Back to the article index
Table of Contents
- ABSTRACT
- 1.INTRODUCTION
- 2.AN INTRODUCTION TO THE DATA
- 3.BASIC PRINCIPLES
- 3.1.Some Nomenclature
- 3.2.Circular Lenses
- 3.3.Non-Circular Lenses
- 4.THE MASS DISTRIBUTIONS OF GALAXIES
- 4.1.Common Models for the
Monopole
- 4.2.The Effective Single Screen
Lens
- 4.3.Constraining the Monopole
- 4.4.The Angular Structure of
Lenses
- 4.5.Constraining Angular
Structure
- 4.6.Model Fitting and the Mass
Distribution of Lenses
- 4.7.Non-Parametric Models
- 4.8.Statistical Constraints on
Mass Distributions
- 4.9.Stellar Dynamics and Lensing
- 5.TIME DELAYS
- 5.1.A General Theory of Time
Delays
- 5.2.Time Delay Lenses in Groups
or Clusters
- 5.3.Observing Time Delays and
Time Delay Lenses
- 5.4.Results: The Hubble Constant
and Dark Matter
- 5.5.The Future of Time Delay
Measurements
- 6.GRAVITATIONAL LENS STATISTICS
- 6.1.The Mechanics of Surveys
- 6.2.The Lens Population
- 6.3.Cross Sections
- 6.4.Optical Depth
- 6.5.Spiral Galaxy Lenses
- 6.6.Magnification Bias
- 6.7.Cosmology With Lens
Statistics
- 6.8.The Current State
- 7.WHAT HAPPENED TO THE CLUSTER
LENSES?
- 7.1.The Effects of Halo Structure
and the Power Spectrum
- 7.2.Binary Quasars
- 8.THE ROLE OF SUBSTRUCTURE
- 8.1.Low Mass Dark Halos
- 9.THE OPTICAL PROPERTIES OF LENS
GALAXIES
- 9.1.The Interstellar Medium of
Lens Galaxies
- 10.EXTENDED SOURCES AND QUASAR HOST
GALAXIES
- 10.1.An Analytic Model for
Einstein Rings
- 10.2.Numerical Models of
Extended Lensed Sources
- 10.3.Lensed Quasar Host Galaxies
- 11.DOES STRONG LENSING HAVE A
FUTURE?
- REFERENCES