Reducing the shear

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dc.creatorWhite, Martin
dc.date2005-01-31
dc.date.accessioned2026-07-07T11:57:09Z
dc.date.available2026-07-07T11:57:09Z
dc.descriptionAs gravitational lensing measurements become increasingly precise, it becomes necessary to include ever higher order effects in the theoretical calculations. Here we show how the difference between the shear and the reduced shear manifest themselves in a number of commonly used measures of shear power. If we are to reap the science rewards of future, high precision measurements of cosmic shear we will need to include this effect in our theoretical predictions.
dc.description9 pages, 5 figures. To appear in Astroparticle Physics
dc.identifierhttps://arxiv.org/abs/astro-ph/0502003
dc.identifierhttp://arxiv.org/abs/astro-ph/0502003
dc.identifierAstropart.Phys.23:349-354,2005
dc.identifierdoi:10.1016/j.astropartphys.2005.01.008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205782
dc.subjectAstrophysics
dc.titleReducing the shear
dc.typetext

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