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J.D. Cohn (UC Berkeley), K. Kadota (Fermilab)
Large SZ selected galaxy cluster surveys are beginning imminently. We compare the dependence of the galaxy cluster angular power spectrum on different modeling assumptions and quantify the tradeoff between depth and area of surveys for its measurement. We also identify the scaling behavior of the cluster angular power spectrum with respect to \sigma8.
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Bulletin of the American Astronomical Society, 36 5
© 2004. The American Astronomical Society.