Window Function for Non-Circular Beam CMB Anisotropy Experiment

Details Window Function for Non-Circular Beam CMB Anisotropy Experiment Window Function for Non-Circular Beam CMB Anisotropy Experiment

2001-05-16

arxiv.org/abs/astro-ph/0105270v1

Astrophys.J. 560 (2001) 28

Astronomy and Astrophysics

Astrophysics

27 pages, 5 figures

Scientific paper

10.1086/322425

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.

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