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Terapixel Surveys for Cosmic Shear | Y. Mellier
; L. van Waerbeke
; M. Radovich
; E. Bertin
; M. Dantel-Fort
; J.-C. Cuillandre
; H. Mc Cracken
; O. Le Fevre
; P. Didelon
; B. Morin
; R. Maoli
; T. Erben
; F. Bernardeau
; P. Schneider
; B. Fort
; B. Jain . ( IAP Paris
; Obs. Paris
; CITA Toronto
; OAC Naples
; CFHT
; Kamuela Hawaii
; LAS Marseille
; SAp
; CE Saclay
; Univ. Roma Sapienza
; Rome
; MPA Garching
; SPhT CE Saclay
; Univ. Bonn
; | Date: |
4 Dec 2000 | Subject: | astro-ph | Affiliation: | 1,2), L. van Waerbeke (3,1), M. Radovich (4,1), E. Bertin (1,2), M. Dantel-Fort, J.-C. Cuillandre, H. Mc Cracken, O. Le Fevre, P. Didelon, B. Morin, R. Maoli(8,1,2), T. Erben, F. Bernardeau(10), P. Schneider(11), B. Fort, B. Jain(12). ( IAP Paris, Ob | Abstract: | The recent detections of cosmic shear signal announced by several groups have demonstrated the feasibility of this challenging program and convinced astro- nomers of its potential for cosmology. Cosmic shear analysis demands to handle Gigabytes of data in order to probe several square degrees in subarcsecond deep imaging mode. The success of these surveys is sensitive to the designs of the observation strategy, the organization of the data reduction pipelines and the links of the data base with surveys like X-ray or spectroscopic follow up. We describe the cosmic shear surveys we have carried out at the VLT and at CFHT and the way we handle this huge data set in a more general context including the VIRMOS and the XMM-LSS surveys, and the future CMB surveys. | Source: | arXiv, astro-ph/0012059 | Services: | Forum | Review | PDF | Favorites |
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