Translator Disclaimer
21 September 2012 VIS: the visible imager for Euclid
Author Affiliations +
Euclid-VIS is a large format visible imager for the ESA Euclid space mission in their Cosmic Vision program, scheduled for launch in 2019. Together with the near infrared imaging within the NISP instrument it forms the basis of the weak lensing measurements of Euclid. VIS will image in a single r+i+z band from 550-900 nm over a field of view of ~0.5 deg2. By combining 4 exposures with a total of 2240 sec, VIS will reach to V=24.5 (10σ) for sources with extent ~0.3 arcsec. The image sampling is 0.1 arcsec. VIS will provide deep imaging with a tightly controlled and stable point spread function (PSF) over a wide survey area of 15000 deg2 to measure the cosmic shear from nearly 1.5 billion galaxies to high levels of accuracy, from which the cosmological parameters will be measured. In addition, VIS will also provide a legacy imaging dataset with an unprecedented combination of spatial resolution, depth and area covering most of the extra-Galactic sky. Here we will present the results of the study carried out by the Euclid Consortium during the Euclid Definition phase.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mark Cropper, R. Cole, A. James, Y. Mellier, J. Martignac, A.-M. Di Giorgio, S. Paltani, L. Genolet, J.-J. Fourmond, C. Cara, J. Amiaux, P. Guttridge, D. Walton, P. Thomas, K. Rees, P. Pool, J. Endicott, A. Holland, J. Gow, N. Murray, L. Duvet, J.-L. Augueres, R Laureijs, P. Gondoin, T. Kitching, R. Massey, and H. Hoekstra "VIS: the visible imager for Euclid", Proc. SPIE 8442, Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave, 84420V (21 September 2012);


VIS: the visible imager for Euclid
Proceedings of SPIE (August 02 2014)
VIS: the visible imager for Euclid
Proceedings of SPIE (July 19 2016)
The focal plane instrumentation for the DUNE mission
Proceedings of SPIE (July 12 2008)
VIS: the visible imager for Euclid
Proceedings of SPIE (August 05 2010)
Sensitivity model for the wide-field infrared explorer mission
Proceedings of SPIE (September 29 1995)
Gaia's FPA: sampling the sky in silicon
Proceedings of SPIE (September 21 2012)

Back to Top