Large Scale Structure: Tracks and Traces
The Table of Contents for the book is as follows:
Preface
List of Participants
I. Galaxy Formation and Evolution
Galaxies at High Redshifts
First Results of the Calar Alto Deep Imaging Survey
Seeing Red: Extremely Red Objects from the Cadis K′ Survey
Luminous Cluster Ellipticals as Cosmological Standard Rods?
HII Galaxies as Tracers of the Mass Distribution in the Nearby Universe
On the Theory of the Cosmological Mass Function
The Twofold Quasar-Galaxy Connection
Effects of Dynamical Friction on the Evolution of the Intracluster Medium
The Cores of Dark Matter Dominated Galaxies: Theory vs. Observations
The Structure of Cold Dark Matter Halos
A Model of the Dark Matter Distribution
Galaxy Tracers in Cosmological N-Body Simulations
Numerical Simulations of Galaxy Formation: Cooling, Heating, Star Formation
Self-Regulating Galaxy Formation: A Numerical Study on the Origin of Galaxy Properties
Star Formation in Cosmological Simulations
High Energy Cosmic Rays and Baryonic Fraction of the Universe
II. Quasar Absorption Lines
Clustering and Large Scale Structure in QSO Absorption
Cosmology from the Structure of the Lyα Forest
QSO Absorption Lines as Chronicle of the Structure Formation History
Clustering Properties of Lyα Absorption Lines in Numerical Simulations
Testing Cosmological Models Using Damped Lyman Alpha Absorbers
III. Galaxy Redshift Surveys
The Two-degree Field (2dF): A Progress Report
The 2dF Galaxy Redshift Survey: Preliminary Results
Cosmology with the SLOAN Digital Sky Survey
Groups of Galaxies in the Las Campanas Redshift Survey
Spatial Correlation Function and Pairwise Velocity Dispersion of Galaxies: CDM Models versus the Las Campanas Survey
Pairwise Velocity Distribution of Galaxies in the Las Campanas Survey
Galaxy Luminosity Segregation Derived from Las Campanas — EDSGC Cross-Correlation Function
A New Large Catalog of Groups of Galaxies in the Southern Galactic Hemisphere
Large Scale Structure from Radio Surveys
ΩM and the CNOC Surveys
Peculiar Motions as Distance Indicators: Reconstruction of the Local Galaxy Density
The Puzzling Structure of the Shapley Supercluster
Cosmological Studies with ASCA Observations of Shapley Supercluster
Large Groups in the Chile-UK Quasar Survey
Significance of Cosmological Redshift Distortions in Future Redshift Surveys of Galaxies
IV. Galaxy Clusters
Tracing the Universe with Clusters of Galaxies
Current Status of the ACO Cluster Redshift Compilation
The Mass Function of Nearby Galaxy Clusters
Calibration of the Mass–Temperature Relation for Clusters of Galaxies
The Nature of the Large Scale Extended X-Ray Emission around Abell Clusters
The Lx – T Correlation for Distant Galaxy Clusters
The Abundance of X-ray Clusters out to z ≃ 0.8
Cosmological Constraints from the ROSAT Deep Cluster Survey
Clusters in Various Cosmological Models: Abundance and Evolution
Properties of Galaxy Clusters
Connecting Large Scale Structure and Cluster Formation
Cluster-Galaxy Correlation Functions in COBE Normalized CDM Models
The Power Spectrum of Clusters of Galaxies
Regularity of the Large Scale Structure of the Universe
Regularity in the Distribution of Superclusters
Minkowski Functionals in Cosmology: An Overview
Characterizing Cluster Morphology Using Vector-Valued Minkowski Functionals
The X-Ray Cluster Dipole
Large Scale Coherent Dipole Anisotropy?
V. Large Scale Structure
Velocity Fields Statistics and Tessellation Techniques: Unbiased Estimators of Ω
Voronoi Tesselations for Statistical Evaluation of Galaxy Distributions
Spherical Harmonic Analysis of Redshift Space Distortions in the IRAS PSCZ Redshift Survey
Power Spectrum of Velocity Fluctuations in the Universe
Statistical Analysis of the Galaxy Peculiar Velocity Field
Variational Dynamics and the Mass of the Local Group
Kinematical Evolution of the Pairwise Velocity Field of Galaxies
Reconstructing Nonlinear Stochastic Bias from Velocity Space Distortions
Measuring the Clustering of Faint Galaxies
N-Point Correlation Functions from the Muenster Redshift Project 2D Catalogue
Scale-Invariant Correlation Functions of Cosmological Density Fluctuations in the Strong Clustering Regime
The Evolution of Galaxy Clustering
Galaxy Clustering at High Redshift
Evolution of Galaxy Clustering
The Evolution of the Two-Points Correlation Function
Early LSS Formation and Quasar Groups
Early Evolution of Large Scale Structure Traced by Faint Blue Galaxies
Mixed Models with n > 1 and Large Scale Structure Constraints
Large Scale Structure Formation in Mixed Dark Matter Models with a Cosmological Constant
The Distribution of Matter in the VIRGO Simulations
Identifying and Quantifying the Tracers of Large Scale Structure: Filaments and Voids
Measures of Walls, Filaments and Voids
Superlarge Scale Structure in the Universe
Large Scale Structure as Cosmological Probe
Alignment of Primordial Density Perturbations as Tracers of Today's Filaments
Accuracy of Nonlinear Approximations in Spheroidal Collapse — Why are Zel'dovich-type Approximations so Good? —
A Fresh Look at the Adhesion Approximation
VI. Gravitational Lensing
Gravitational Lensing as a Cosmological Probe
Weak Gravitational Lensing: Correlations for Open and Flat Models
Weak Lensing of QSOs by the Large Scale Structure
QSO-Galaxy Correlations Induced by Weak Lensing
The Cosmological Uncertainty Principle
The Δθ-zs Relation as a Cosmological Test
On Arcs and Ω
The Edge-on Spiral Gravitational Lens B1600+434
A Search for Large Image Separation Gravitational Lenses in the JVAS Radio Survey
Limits on MACHOs in the Lensing Galaxy 0957+561
Cluster Mass Estimation from Lens Magnification
Cluster Mass Profiles from Lensing
Do Cluster Galaxies Have Extended Dark Halos?
VII. Cosmic Background Radiation and Inflation
A Brief Overview of the Scientific Capabilities of MAP and Planck
Cosmological Evolution of X–Ray AGN
Large Angular Scale Fluctuations in the X-Ray Background
The Tophat and MASM CMB Experiments: Status
Evidence of a Built-in Scale on the Primeval Matter Power Spectrum
Cosmic Background Maps of Primordial Voids
Inflation for Large Scale Structure
Inflationary Models with Λ-Term and CMB Anisotropy
New Steps Towards a Proof of the Cosmological “No Hair” – Theorem
Concluding Remarks
Author Index