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Article Contents
- ABSTRACT
- 1.INTRODUCTION
- 2.MODELS OF THE GALAXY-HALO
CONNECTION
- 2.1.Preliminaries: What is a
halo?
- 2.2.Empirical models of the
galaxy-halo connection
- 2.3.Physical models of galaxy
formation
- 2.4.Complementarity between
approaches
- 3.MEASUREMENTS THAT INFORM THE
GALAXY-HALO CONNECTION
- 3.1.Galaxy abundance
- 3.2.Two-point galaxy clustering
- 3.3.Group and cluster catalogs
- 3.4.Weak gravitational lensing
- 3.5.Additional observables
- 4.BEYOND THE SIMPLEST MODELS OF THE
GALAXY-HALO CONNECTION
- 4.1.What halo property is best
matched to galaxies?
- 4.2.What galaxy property is best
matched to halos?
- 4.3. Scatter
- 4.4.Assembly bias
- 4.5. Centrals vs. Satellites
- 4.6.Occupation properties of
satellite galaxies
- 4.7. Joint modeling of mass and
secondary properties
- 5.CURRENT CONSTRAINTS ON THE
GALAXY-HALO CONNECTION AS EXPRESSED BY THE SHMR
- 5.1.The mean stellar-to-halo
mass relation for central galaxies
- 5.2. Scatter for central
galaxies
- 5.3.Evolution
- 5.4.How does assembly bias manifest
observationally?
- 5.5.Systematic uncertainties
- 6.CURRENT CONSTRAINTS ON SECONDARY
PROPERTIES IN THE GALAXY-HALO CONNECTION
- 6.1.Stellar-to-Halo Mass
Relations for star-forming and passive central galaxies
- 6.2.How does assembly bias manifest
observationally for secondary properties?
- 6.3.Why do galaxy properties
depend on environment?
- 6.4.Galaxy Sizes
- 7.APPLICATIONS OF THE GALAXY-HALO
CONNECTION
- 7.1.Understanding the Physics
of Galaxy Formation
- 7.2.Inferring Cosmological
Parameters
- 7.3.Probing the Properties and
Distribution of Dark Matter
- 8.STATUS AND OUTLOOK
- REFERENCES