Constraining the Power Spectrum Using the Column Density Distribution: a Status Report

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dc.creatorHui, Lam
dc.date1997-12-04
dc.date.accessioned2026-07-07T02:25:29Z
dc.date.available2026-07-07T02:25:29Z
dc.descriptionWe review the arguments for how the slope of the column density distribution of the Lyman-alpha forest should depend on the matter power spectrum. The latest progress, presented by various groups in this conference and elsewhere, is summarized.
dc.description6 pages Latex, 1 ps fig, to appear in the Proc. of the 13th IAP Colloquium: Structure and Evolution of the IGM from QSO Absorption Line Systems, eds. P. Petitjean and S. Charlot
dc.identifierhttps://arxiv.org/abs/astro-ph/9712075
dc.identifierhttp://arxiv.org/abs/astro-ph/9712075
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11896
dc.subjectAstrophysics
dc.titleConstraining the Power Spectrum Using the Column Density Distribution: a Status Report
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