Window function for non-circular beam CMB anisotropy experiment

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dc.contributor.authorSouradeep, Tarun
dc.contributor.authorRatra, Bharat
dc.date.accessioned2012-03-13T11:03:05Z
dc.date.available2012-03-13T11:03:05Z
dc.date.issued2001-07-05
dc.description.abstractWe 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.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1444
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprint;22/01
dc.subjectCosmic microwave backgrounden_US
dc.subjectCosmology: theoryen_US
dc.subjectMethods: analyticalen_US
dc.subjectMethods: data analysisen_US
dc.titleWindow function for non-circular beam CMB anisotropy experimenten_US
dc.typeArticleen_US

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