Cosmological Parameters from Spherical Harmonic Analyses

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dc.creatorScharf, Caleb. A.
dc.date1993-09-20
dc.date.accessioned2026-07-07T02:18:52Z
dc.date.available2026-07-07T02:18:52Z
dc.descriptionIn the rest of this volume Lahav and Fisher have presented the method of Spherical Harmonic Analysis (SHA) and its use in estimating cosmologically interesting parameters. Here I demonstrate the use of SHA in cross-correlating galazy catalogues and present an estimate of the ratio of the optical and IRAS galaxy bias parameters; b_O/b_I ~ 1.7.
dc.descriptionParis Conference 2 pages uuencoded postscript file- figure available upon request
dc.identifierhttps://arxiv.org/abs/astro-ph/9309031
dc.identifierhttp://arxiv.org/abs/astro-ph/9309031
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9656
dc.subjectAstrophysics
dc.titleCosmological Parameters from Spherical Harmonic Analyses
dc.typetext

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