Window Function for Non-Circular Beam CMB Anisotropy Experiment
arXiv:astro-ph/0105270 · doi:10.1086/322425
Abstract
We develop computationally rapid methods to compute the window function for a cosmic microwave background anisotropy experiment with a non-circular beam which scans over large angles on the sky. To concretely illustrate these methods we compute the window function for the Python V experiment which scans over large angles on the sky with an elliptical Gaussian beam.
27 pages, 5 figures
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