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Akademický článek
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Akademický článek
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Autor:
P. Sanchez, Anne Costille, C. Pariès, S. Tisserand, C. Rossin, Y. Salaun, B. Foulon, T. Weber, A. Caillat, Sandrine Pascal
Publikováno v:
International Conference on Space Optics — ICSO 2018.
The launch of ESA EUCLID mission is foreseen in 36020. The goal of the mission is to understand the nature of the dark energy and to map the geometry of the dark matter. The EUCLID telescope will be equipped with two instruments working in the visibl
Autor:
P. Sanchez, C. Pariès, C. Rossin, Sandrine Pascal, B. Foulon, Rudy Barette, Anne Costille, A. Caillat, Philippe Laurent
Publikováno v:
Proc.SPIE Int.Soc.Opt.Eng.
SPIE Astronomical Telescopes + Instrumentation 2018
SPIE Astronomical Telescopes + Instrumentation 2018, Jun 2018, Austin, United States. pp.106982B, ⟨10.1117/12.2309493⟩
SPIE Astronomical Telescopes + Instrumentation 2018
SPIE Astronomical Telescopes + Instrumentation 2018, Jun 2018, Austin, United States. pp.106982B, ⟨10.1117/12.2309493⟩
International audience; ESA EUCLID mission will be launched in 2020 to understand the nature of the dark energy responsible of the accelerated expansion of the Universe and to map the geometry of the dark matter. The map will investigate the distance
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2a3d415cf39852c8a5ab545a2712ba7d
https://hal.archives-ouvertes.fr/hal-01871660
https://hal.archives-ouvertes.fr/hal-01871660
Publikováno v:
International Conference on Space Optics — ICSO 2016.
Dark matter and dark energy mysteries will be explored by the Euclid ESA M-class space mission which will be launched in 2020. Millions of galaxies will be surveyed through visible imagery and NIR imagery and spectroscopy in order to map in three dim
Autor:
A. Vasseur, E. Lagneau, N. Lescut, B. Foulon, B. Schipman, A. Lépinoy, J.Y. Gosselin, P. Lamoly
Publikováno v:
Physica Medica. 56:43
Introduction As part of the service quality assurance program, the implementation of 4D imaging required the implementation of a new quality control. The main idea was to evaluate the restitution of the shape, volume and position of a moving object t
Publikováno v:
SPIE Proceedings.
The Euclid space mission aims at elucidating dark matter and dark energy mysteries thanks to two scientific instruments: VIS, the visible camera and NISP, the Near Infrared Spectro-Photometer. Millions of galaxies spectra will be recorded thanks to i
Autor:
Serge Reynaud, J. H. Hough, P. d'Arrigo, C. Jentsch, B. Lamine, John Mester, John D. Barrow, H. Ward, H. Dittus, Ulrich Johann, J. T. Mendonça, Markus Arndt, C. Trenkel, G. D. Hammond, G. Amelino-Camelia, Martin E. Caldwell, F. Loeffler, Stefano Vitale, Chen Wang, Philippe Bouyer, H. A. Klein, C.M. Pegrum, Ernst M. Rasel, Astrid Lambrecht, Robert Bingham, C. I. Torrie, W. Vodel, Claus Lämmerzahl, Thibault Damour, N. A. Lockerbie, Patrick Gill, B. Foulon, D. Shaul, A. Woodgate, T. J. Sumner, A. M. Cruise, Wei-Tou Ni, Ch.J. Bordé, Wolfgang Ertmer, Karen Aplin, Stephan Theil, Pierre Touboul, Philippe Jetzer, Achim Peters
Publikováno v:
Experimental Astronomy
Experimental Astronomy, springer Link, 2009, 23, pp.549-572. ⟨10.1007/s10686-008-9086-9⟩
Experimental Astronomy, 2009, 23, pp.549-572. ⟨10.1007/s10686-008-9086-9⟩
Experimental Astronomy, springer Link, 2009, 23, pp.549-572. ⟨10.1007/s10686-008-9086-9⟩
Experimental Astronomy, 2009, 23, pp.549-572. ⟨10.1007/s10686-008-9086-9⟩
The GAUGE (GrAnd Unification and Gravity Explorer) mission proposes to use a drag-free spacecraft platform onto which a number of experiments are attached. They are designed to address a number of key issues at the interface between gravity and unifi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6994aa5e96b7f45b149719bcaff3541a
https://ora.ox.ac.uk/objects/uuid:9a9d2391-673b-41dc-874d-04be53098fab
https://ora.ox.ac.uk/objects/uuid:9a9d2391-673b-41dc-874d-04be53098fab
Publikováno v:
SPIE Proceedings.
ESA Euclid mission is designed to map the geometry of the dark Universe. The NISP (Near Infrared Spectro- Photometer) is one of its two instruments dedicated to NIR with two main observing modes: the photometric mode and the spectroscopic mode, for t
Autor:
Eric Prieto, B. Foulon, W. Ceria, Tony Pamplona, Didier Castel, A. Febvre, Michel Bougoin, Thierry Maciaszek, Jean-Luc Gimenez, Franck Ducret, Laurent Martin
Publikováno v:
SPIE Proceedings.
In the scope of EUCLID spatial mission, NISP instrument requires high positioning accuracy and high dimensional stability to achieve the required optical performances. LAM is in charge of the development of the instrument main structure which is base