James Webb Space Telescope optical simulation testbed IV: linear control alignment of the primary segmented mirror and the secondary mirror

Author(s):  
Sylvain Egron ◽  
Rémi Soummer ◽  
Vincent Michau ◽  
Aurelie Bonnefois ◽  
Marc Ferrari ◽  
...  
Author(s):  
Charles-Philippe Lajoie ◽  
Aurélie Bonnefois ◽  
Lucie Leboulleux ◽  
Laurent Pueyo ◽  
Marie Ygouf ◽  
...  

2016 ◽  
Author(s):  
Sylvain Egron ◽  
Charles-Philippe Lajoie ◽  
Lucie Leboulleux ◽  
Mamadou N'Diaye ◽  
Laurent Pueyo ◽  
...  

2014 ◽  
Author(s):  
Élodie Choquet ◽  
Olivier Levecq ◽  
Mamadou N'Diaye ◽  
Marshall D. Perrin ◽  
Rémi Soummer

2014 ◽  
Author(s):  
Marshall D. Perrin ◽  
Rémi Soummer ◽  
Élodie Choquet ◽  
Mamadou N'Diaye ◽  
Olivier Levecq ◽  
...  

2007 ◽  
Vol 3 (S250) ◽  
pp. 491-494
Author(s):  
George Sonneborn

AbstractThe James Webb Space Telescope (JWST) is a large, infrared-optimized space telescope scheduled for launch in 2013. JWST will find the first stars and galaxies that formed in the early universe, connecting the Big Bang to our own Milky Way galaxy. JWST will peer through dusty clouds to see stars forming planetary systems, connecting the Milky Way to our own Solar System. JWST's instruments are designed to work primarily in the infrared range of 1 - 28 μm, with some capability in the visible range. JWST will have a large segmented mirror, ~6.5 m in diameter, and will be diffraction-limited at 2 μm (< 0.1 arcsec resolution). JWST will be placed in an L2 orbit about 1.5 million km from the Earth. The instruments will provide imaging, coronography, and multi-object and integral-field spectroscopy across the 1 - 28 μm wavelength range. The breakthrough capabilities of JWST will enable new studies of massive stars from the Milky Way to the early universe.


2003 ◽  
Author(s):  
Alfred B. Schultz ◽  
Richard G. Lyon ◽  
Mark Kochte ◽  
Dorothy A. Fraquelli ◽  
Frederick Bruhweiler ◽  
...  

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