Detection of Cosmic Shear with the William Herschel Telescope

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dc.creatorBacon, David
dc.creatorRefregier, Alexandre
dc.creatorEllis, Richard
dc.date2000-08-16
dc.date.accessioned2026-07-07T01:54:57Z
dc.date.available2026-07-07T01:54:57Z
dc.descriptionGravitational lensing by large-scale structure induces weak coherent alignments in the shapes of background galaxies. Here we present evidence for the detection of this `cosmic shear' at the 3.4 sigma significance level with the William Herschel Telescope. Analysis and removal of notable systematic effects, such as shear induced by telescope optics and smearing by tracking and seeing, are conducted in order to recover the physical weak shear signal. Positive results for shear recovery on realistic simulated data are presented, enhancing confidence in the measurement method. The detection of cosmic shear is statistically characterised, and its cosmological significance is discussed.
dc.description4 pages, including 3 figures. To appear in Proceedings of XXth Moriond Astrophysics Meeting, "Cosmological Physics with Gravitational Lensing", eds. J.-P. Kneib, Y. Mellier, M. Moniez and J. Tran Thanh Van
dc.identifierhttps://arxiv.org/abs/astro-ph/0008248
dc.identifierhttp://arxiv.org/abs/astro-ph/0008248
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1490
dc.subjectAstrophysics
dc.titleDetection of Cosmic Shear with the William Herschel Telescope
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