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Displaying 49 authors out of 49
A. FERRARA (SISSA, Trieste, Italy)
Cosmological Radiative Transfer: Where Do We Stand?
A. SLOSAR (University of Ljubljana, Slovenia)
Recent Advances in Model Comparison Techniques
A.E. EVRARD (The University of Michigan, Ann Arbor, U.S.A.)
Precise Observable-Mass Relations for Clusters of Galaxies
B. CIARDI (Max-Planck-Institute for Astrophysics, Garching, Germany)
Modeling Radiative Transfer in Simulations of Cosmic Reionization
B. METCALF (University of California, Santa Cruz, U.S.A.)
Simulating Strong Gravitational Lenses and their Small-Scale Structure
B.D. WANDELT (University of Illinois at Urbana-Champaign, U.S.A.)
New Techniques for Analyzing Cosmological Data Sets
C. PARK (Korea Institute for Advanced Study, Seoul, Korea)
Theoretical and Observational Studies of Topology of Large Scale Structure
C.M. HIRATA (Princeton University, New Jersey, U.S.A.)
A Fast Method for Likelihood Evaluations
C.S. FRENK (Institute for Computational Cosmology, Durham, U.K.)
The Crucial Effects of Feedback in Semi-Analytic Models and Numerical Simulations of Galaxy Formation
D. MERRITT (Rochester Institute of Technology, U.S.A.)
Beyond the Million-Body Problem: Simulating Galactic Nuclei
D. RYU (Chungnam National University, Daejeon, Korea)
Shock Waves and Shock-Heated Gas in Gosmological Hydrodynamic Simulations
D.J. CROTON (Max-Planck-Institute for Astrophysics, Garching, Germany)
The Influence of AGN Feedback on Galaxy Properties
E. PIERPAOLI (California Institute of Technology, Pasadena, U.S.A.)
Galaxy Clusters and Ultra-High Energy Cosmic Rays
E. RIPAMONTI (Kapteyn Astronomical Institute, Groningen, The Netherlands)
Numerical Investigations of the Formation of the First Stars
E.J. HAYASHI (Max-Planck-Institute for Astrophysics, Garching, Germany)
Mass Distribution in Cluster Halos
F. GOVERNATO (University of Washington, Seattle, U.S.A.)
Better, Stronger, Faster: Effects of Feedback on Galaxy Formation
G. FARRAR (New York University, U.S.A.)
Large Scale Magnetic Structure Elucidated by a Cluster of UHE Cosmic Rays
G. TORMEN (Università degli Studi di Padova, Italy)
Views of Galaxy Clusters
G.M. VOIT (Michigan State University, Ann Arbor, U.S.A.)
A Framework for AGN Feedback in Cluster Cores
H. TRAC (Princeton University, New Jersey, U.S.A.)
Hydrodynamic Simulations of the Lyman Alpha Forest
I.T. ILIEV (University of Toronto (CITA), Ontario, Canada)
A New Photon-Conserving Method for Cosmological Radiative Transfer
J. BINNEY (Rudolf Peierls Centre for Theoretical Physics, Oxford, U.K.)
How AGN Terminate Galaxy Formation
J. DIEMAND (University of California, Santa Cruz, U.S.A.)
Density Profiles and Substructure: Approximating CDM Halos with N-Body Models
J.F. NAVARRO (University of Victoria, British Colombia, Canada)
The Accretion History of the Milky Way
J.S. BAGLA (Harish-Chandra Research Institute, Allahabad, India)
The Adaptive TreePM Method
K. DOLAG (Max-Planck-Institute for Astrophysics, Garching, Germany)
The Quest for Cluster Simulations
L. GAO (Max-Planck-Institute for Astrophyiscs, Garching, Germany)
Early Structure in LCDM Universe
L.-L. FENG (Purple Mountain Observatory, Nanjing, P.R. of China)
The Fast Algorithm of Clustering Statistics for a Large Data Set
L.-M. CHENG (Institute of Theoretical Physics, Beijing, P.R. of China)
Stimulating the Soft X-Ray Excess in Clusters of Galaxies
M. DORAN (Universität Heidelberg, Germany)
Speeding up Cosmological Boltzmann Codes
M. JOYCE (Universite de Paris VI, France)
Quantifying Discreteness Effects in Cosmological N Body Simulations
M. VIEL (University of Cambridge, U.K.)
The Lyman-Alpha Forest as a Cosmological Probe
P. COLIN (Universidad Nacional Autonoma de Mexico, Michoacan, Mexico)
The Dependence on Environment of Cold Dark Matter Halos
P. MCDONALD (University of Toronto (CITA), Ontario, Canada)
Cosmology from the Lyman-Alpha Forest
P. TISSERA (Instituto de Astronomia y Fisica del Espacio, Buenos Aires, Argentina)
SN Feedback and Galaxy Formation
P.A. THOMAS (University of Sussex, Brighton, U.K.)
Cluster Formation and Evolution
R. SCOCCIMARRO (New York University, U.S.A.)
Large-Scale Structure beyond the Power Spectrum
R. TEYSSIER (Service d'Astrophysics CEA, Gif-sur-Yvette, France)
Galaxy Formation with Adaptive Mesh Refinement
R.J. BOND (University of Toronto (CITA), Ontario, Canada)
Computational Issues in CMB Analysis, Now and Then
S. BORGANI (Università degli Studi di Trieste, Italy)
Studying Galaxy Clusters with Hydrodynamical Simulations
S. WHITE (Max-Planck-Institute for Astrophyiscs, Garching, Germany)
Gas Accretion during Galaxy Assembly
T. DI MATTEO (Carnegie Mellon University, Pittsburgh, U.S.A.)
The Self-Regulated Growth of Black Holes during Galaxy Collisions
T.R. CHOUDHURY (SISSA, Trieste, Italy)
Observational Constraints on Self-Consistent Reionization Models
T.R. QUINN (University of Zurich, Switerland)
Star Formation in Simulations of Galaxy Formation
U. SELJAK (ICTP, Trieste, Italy)
Halo Model Versus Simulations
U.-L. PEN (University of Toronto (CITA), Ontario, Canada)
A Fast Parallel PM Code
V. SPRINGEL (Max-Planck-Institute for Astrophysics, Garching, Germany)
The Universe in a Supercomputer: From the First Quasars to the Large-Scale Galaxy Distribution
Y. JING (Shanghai Astronomical Observatory, P.R. of China)
Galaxy Formation and Strong Lensing
Y. SUTO (The University of Tokyo, Japan)
Searching for Emission and Absorption Signatures of Warm/Hot Intergalactic Medium with DIOS (Diffuse Intergalactic Oxygen Surveyor): Mock Observation of Cosmological Simulation Data

Organizers

A. Ferrara, Y. Jing, U.-L. Pen, U. Seljak, S. White