DescriptionGalaxy clusters have played a crucial role in the development of modern cosmology over the past century. Thanks to the next generation of high resolution microwave telescopes, a new generation of cluster surveys (detected through the Sunyaev-Zel'dovich (SZ) effect) are under way and promise to provide us with a catalog of hundreds to thousands of new high redshift clusters over the next few years. This conference aims to bring together experts in SZ observations and cluster cosmology to understand the status/implications of current clusters surveys, and find a consensus on the future promise/prospects of cosmology with galaxy clusters.
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The Shape of Clusters and Large-Scale Structure
Neta Bahcall Princeton University
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Clusters of Galaxies in Microwave and X-Ray Spectral Bands
Rashid Sunyaev Max-Planck-Institut für Astrophysik (MPA), Garching
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The Red-Sequence Cluster Survey and its Applications to Cosmology
Howard Yee University of Toronto
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The Stellar Components of Nearby Galaxy Clusters
Dennis Zaritsky University of Arizona
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Optimal Filtering: A Real-World Example
Tom Crawford University of Chicago
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The APEX Sunyaev Zel'dovich Experiment Observations
Matt Dobbs McGill University
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Characterizing the SPT cluster selection function
Laurie Shaw McGill University
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Sharpening the Precision of SZ Studies
Gilbert Holder University of Illinois Urbana-Champaign