paper

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

References in corpus (5)

Cited by in corpus (33)