Understanding the Optimal Redshift Range for the Supernovae Hubble Diagram

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dc.creatorLinder, Eric V.
dc.date2001-08-16
dc.date.accessioned2026-07-07T01:59:40Z
dc.date.available2026-07-07T01:59:40Z
dc.descriptionThe supernovae Hubble diagram traces the expansion history of the universe, including the influence of dark energy. Its use to probe the cosmological model can fruitfully be guided by heuristic study of the features of the model curves. By relating these directly to the physics of the expansion we can understand simply the optimal redshift range for supernovae observations, requiring a survey depth of z=1.5-2 to distinguish evolution in dark energy properties.
dc.description14 pages, 6 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0108280
dc.identifierhttp://arxiv.org/abs/astro-ph/0108280
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3207
dc.subjectAstrophysics
dc.titleUnderstanding the Optimal Redshift Range for the Supernovae Hubble Diagram
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