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Aird, K. K. Schaffer, K. T. Story, K. Vanderlinde, L. E. Bleem, L. Knox, L. M. Mocanu, L. Shaw, M. A. Dobbs, M. Lueker, M. Millea, N. W. Halverson, O. Zahn, R. Keisler, R. Williamson, S. Bhattacharya, S. Hoover, S. Padin, S. S. Meyer, T. de Haan, T. E. Montroy, T. M. Crawford, T. Plagge, W. L. Holzapfel, Z. Hou, Z. Staniszewski","submitted_at":"2013-03-14T18:06:30Z","abstract_excerpt":"We present a measurement of the angular bispectrum of the millimeter-wave sky in observing bands centered at roughly 95, 150, and 220 GHz, on angular scales of $1^\\prime \\lesssim \\theta \\lesssim 10^\\prime$ (multipole number $1000 \\lesssim l \\lesssim 10000$). At these frequencies and angular scales, the main contributions to the bispectrum are expected to be the thermal Sunyaev-Zel'dovich (tSZ) effect and emission from extragalactic sources, predominantly dusty, star-forming galaxies (DSFGs) and active galactic nuclei. 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