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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Heating and Cooling of the Intracluster Medium
Arif Babul University of Victoria
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XRay observations normalized ICM models: SZ scaling relations and cosmological implications
Subha Majumdar Tata Institute of Fundamental Research (TIFR)
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Thermodynamics of Galaxy Clusters and Beyond
Daisuke Nagai Yale University
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The Power of Sunyaev-Zeldovich, Then and Now
Richard Bond Canadian Institute for Theoretical Astrophysics (CITA)
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How non-thermal processes of the intracluster medium affect the Sunyaev-Zeldovich angular power spectrum
Nick Battagalia Canadian Institute for Theoretical Astrophysics (CITA)
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Cosmic Background Imager
Jon Sievers McGill University - Department of Physics
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SZ Calibration with the Sunyaev-Zel'dovich Array
Dan Marrone University of Chicago