Prospects for weak lensing/cosmic shear with VLTs

Bonn); CE Saclay); E. Bertin (IAP; Obs. de Paris/LERMA); F. Bernardeau (SPhT; I. Tereno (IAP; L. van Waerbeke (IAP; CITA); P. Schneider (IAEF; T. Erben (IAEF; Univ. Lisbon); Y. Mellier (IAP; Obs. de Paris/LERMA)

arxiv: astro-ph/0210093 · v1 · submitted 2002-10-03 · 🌌 astro-ph

Prospects for weak lensing/cosmic shear with VLTs

Y. Mellier (IAP; Obs. de Paris/LERMA) , L. van Waerbeke (IAP; CITA) , E. Bertin (IAP; Obs. de Paris/LERMA) , I. Tereno (IAP , Univ. Lisbon) , P. Schneider (IAEF , Bonn) , F. Bernardeau (SPhT

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CE Saclay) T. Erben (IAEF

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classification 🌌 astro-ph

keywords cosmiclensingshearsurveystelescopesweakanalysesclusters

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The present status of weak lensing analyses of clusters of galaxies and of cosmic shear surveys are presented and discussed. We focus on the impact of very large telescopes on present-day and future surveys and compare their potential with HST or wide field 4 meter telescopes.

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Prospects for weak lensing/cosmic shear with VLTs

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