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G. Spieler, H. M. Cho, J. D. Hrubes, J. D. Vieira, J. E. Carlstrom, J. E. Ruhl, J. Hlavacek-Larrondo, J. J. McMahon, J. J. Mohr, J. Liu, J. Mehl, J. P. Dudley, J. Ruel, J. T. Sayre, K. A. Aird, K. K. Schaffer, K. Story, K. Vanderlinde, L. E. Bleem, L. Knox, L. Mocanu, M. A. Dobbs, M. Bayliss, M. Brodwin, M. D. Gladders, M. Lueker, M. McDonald, N. W. Halverson, O. Zahn, R. J. Foley, R. Keisler, R. Williamson, S. A. Stanford, S. Bocquet, S. Desai, S. Padin, S. S. Meyer, S. S. Murray, T. de Haan, T. E. Montroy, T. M. Crawford, W. L. Holzapfel, W. R. Forman, Z. Staniszewski","submitted_at":"2013-12-11T01:16:19Z","abstract_excerpt":"We describe a method for measuring the integrated Comptonization (YSZ) of clusters of galaxies from measurements of the Sunyaev-Zel'dovich (SZ) effect in multiple frequency bands and use this method to characterize a sample of galaxy clusters detected in South Pole Telescope (SPT) data. 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