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Article Contents
- ABSTRACT
- 1.ROLE OF OBSERVATIONS IN COSMOLOGY &
GALAXY FORMATION
- 1.1.The Observational Renaissance
- 1.2.Observations Lead to Surprises
- 1.3.Recent Observational
Milestones
- 1.4.Concordance Cosmology: Why is
such a curious model acceptable?
- 1.5.Lecture Summary
- 2.GALAXIES & THE HUBBLE SEQUENCE
- 2.1.Introduction: Changing Paradigms
of Galaxy Formation
- 2.2.Galaxy Morphology - Valuable Tool
or Not?
- 2.3.Semi-Analytical Modeling
- 2.4.A Test Case: The Galaxy
Luminosity Function
- 2.5.The Role of the Environment
- 2.6.The Importance of High
Redshift Data
- 2.7.Lecture Summary
- 3.COSMIC STAR FORMATION HISTORIES
- 3.1.When Did Galaxies Form? Searches
for Primeval Galaxies
- 3.2.Local Inventory of Stars
- 3.3.Diagnostics of Star Formation
in Galaxies
- 3.4.Cosmic Star Formation -
Observations
- 3.5.Cosmic Star Formation - Theory
- 3.6.Unifying the Various High
Redshift Populations
- 3.7.Lecture Summary
- 4.STELLAR MASS ASSEMBLY
- 4.1.Motivation
- 4.2.Methods for Estimating Galaxy
Masses
- 4.3.Results: Regular Galaxies 0
< z < 1.5
- 4.4.Stellar Masses from
Multi-Color Photometry
- 4.5.Results: Stellar Mass
Functions 0 < z < 1.5
- 4.6.Results: Stellar Mass
Functions z > 1.5
- 4.7.Quiescent Galaxies with 2 <
z < 3
- 4.8.Lecture Summary
- 5.WITNESSING THE END OF COSMIC
REIONIZATION
- 5.1.Introduction - Some Weighty
Questions
- 5.2.The Gunn-Peterson Test and
SDSS QSOs
- 5.3.Metallicity of the High
Redshift IGM
- 5.4.Linear Polarization in the
WMAP Data
- 5.5.Stellar Mass Density at z
5-6
- 5.6.Lecture Summary
- 6.INTO THE DARK AGES: LYMAN DROPOUTS
- 6.1.Motivation
- 6.2.Contamination in z
6 Dropout Samples
- 6.3.Cosmic Variance
- 6.4.Evolution in the UV Luminosity
Density 3 < z < 10?
- 6.5.The Abundance of Star Forming
Sources Necessary for Reionization
- 6.6.The Spitzer Space Telescope
Revolution: Stellar Masses at z
6
- 6.7.Lecture Summary
7.LYMAN ALPHA EMITTERS AND
GRAVITATIONAL LENSING
7.1.Strong Gravitational Lensing -
A Primer
7.2.Creating a Cluster Mass Model
7.3.Lensing in Action: Some High z
Examples
7.4.Lyman alpha Surveys
7.5.Results from Narrow Band
Ly
Surveys
7.6.Results from Lensed
Ly
Surveys
7.7.Lecture Summary
8.COSMIC INFRARED BACKGROUND
8.1.Motivation
8.2.Methodogy
8.3.Recent Background Measurements
8.4.Fluctuation Analyses
8.5.EBL Constraints from TeV Gamma
Rays
8.6.Lecture Summary
9.EPILOGUE: FUTURE PROSPECTS
9.1.Introduction
9.2.The Next Five Years
9.3.Beyond Five Years
REFERENCES