Detection of Cosmic Shear from STIS Parallel Archive Data: Data Analysis

Simple item page
dc.creatorMiralles, J. -M.
dc.creatorHaemmerle, H.
dc.creatorPirzkal, N.
dc.creatorSchneider, P.
dc.creatorErben, T.
dc.creatorFosbury, R. A. E.
dc.creatorFreudling, W.
dc.creatorJain, B.
dc.creatorWhite, S.
dc.date2001-09-26
dc.date.accessioned2026-07-07T02:00:19Z
dc.date.available2026-07-07T02:00:19Z
dc.descriptionIn June 1997, parallel observations using the Space Telescope Imaging Spectrograph (STIS) on the HST started to be taken in substantial numbers along many different lines-of-sight. We are using the imaging data to investigate the distortion of background galaxies by the gravitational field of the large scale matter distribution, also known as Cosmic Shear. This poster presents the data and the catalog production that leads to the cosmic shear result presented in the poster "First Cosmic Shear results from STIS parallel program archive data" (Haemmerle et al., this conference). The data is publicly available also at http://www.stecf.org/projects/shear .
dc.description4 pages, 2 figures, to appear in the proceedings of the STScI 2001 spring symposium "The Dark Universe: Matter, Energy and Gravity" Baltimore April 2-5 2001. Poster in Original format available at http://www.astro.uni-bonn.de/~miralles/Balt_post.htm
dc.identifierhttps://arxiv.org/abs/astro-ph/0109485
dc.identifierhttp://arxiv.org/abs/astro-ph/0109485
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3400
dc.subjectAstrophysics
dc.titleDetection of Cosmic Shear from STIS Parallel Archive Data: Data Analysis
dc.typetext

Files

Collections

arXiv