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CMBFAST

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CMBFAST is a computational code used for calculating the anisotropies in the cosmic microwave background (CMB) radiation. Developed by Uros Seljak and Matias Zaldarriaga in the late 1990s, CMBFAST solves the Boltzmann equations that describe the evolution of the CMB's temperature fluctuations and polarization, among other properties related to the early Universe.

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