Notes from Aspen Cluster Workshop May/June 2003
- May 28
- P. Mazzotta: Cold Fronts in Clusters
- O. Czoske: High Speed Cluster Collisions
- P. Ricker: Not-So-Tiny Bubbles
- C. Scharf: X-ray Observations of Clusters
- M. Meneghetti: Arc Statistics with Cluster Simulations
- G. Tormen: ICM Dynamics
- May 30 morning
- D. Zaritsky: ESO Distant Cluster Survey
- H. Yee: Cosmology with Cluster Surveys
- P. Henry: Cosmology From (mostly) Xray L,T Functions
- S. Majumdar: Future Large Cluster Surveys
- A. Sanderson: Scaling Relations for Clusters
- A. Zabludoff: Galaxy Evolution in Groups and Clusters
- May 30 pm discussion
What is the Best Way To Find Clusters?
- June 2 afternoon
- R. Wechsler: Simulating Cluster Observables
- A. Berlind: Modeling DM Halo Occupation
- R. Sheth: Testing Analytic Halo Models
- A. Kravtsov: The Dark Side of Halo Occupation Distributions
- June 4 morning
- B. Nichol: Galaxy Evolution in Clusters and Groups
- M. Bernardi: Early type galaxies and their environment: constraints on galaxy formation models
- A. Cooray: Transition from Linear to non-linear power spectrum
- L. Moscardini: Modelling the ICM and DM distributions in high-res simulations
- M. Valluri: Substructure in Hydra I cluster (A1060) from HI
- June 4 pm discussion
How Do (Should) Theorists Define Cluster Mass?
- June 5 morning session
- R. Gal: Northern Sky Optical Cluster Survey: Richness=Mass?
- K. Romer: XCS XMM Cluster Survey
- C. Miller: Radial Profiles of Galaxies in Clusters
- Z. Haiman: Using power spectrum to constrain cosmology
Disclaimer: these are notes taken by Roy Gal, and may not accurately reflect the intended meaning of the speakers!