Window Functions for CMB Experiments

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dc.creatorWhite, Martin
dc.creatorSrednicki, Mark
dc.date1994-02-15
dc.date.accessioned2026-07-07T12:01:00Z
dc.date.available2026-07-07T12:01:00Z
dc.descriptionWe discuss the applicability and derivation of window functions for cosmic microwave background experiments on large and intermediate angular scales. These window functions describe the response of the experiment to power in a particular mode of the fluctuation spectrum. We give general formulae, illustrated with specific examples, for the most common observing strategies.
dc.description12 pages in Plain Tex, UCSBTH--94--03, CfPA--94--TH--11
dc.identifierhttps://arxiv.org/abs/astro-ph/9402037
dc.identifierhttp://arxiv.org/abs/astro-ph/9402037
dc.identifierAstrophys.J.443:6,1995
dc.identifierdoi:10.1086/175497
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/206968
dc.subjectAstrophysics
dc.titleWindow Functions for CMB Experiments
dc.typetext

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