Cryogenic filter- and spectrometer wheels for the Mid Infrared Instrument (MIRI) of the James Webb Space Telescope (JWST)

2006 ◽  
Author(s):  
D. Lemke ◽  
A. Böhm ◽  
F. de Bonis ◽  
M. Ebert ◽  
T. Gross ◽  
...  
2016 ◽  
Author(s):  
Sarah Kendrew ◽  
Silvia Scheithauer ◽  
Patrice Bouchet ◽  
Jerome Amiaux ◽  
Ruymán Azzollini ◽  
...  

2008 ◽  
Author(s):  
Kimberly Banks ◽  
Melora Larson ◽  
Cagatay Aymergen ◽  
Burt Zhang

2006 ◽  
Author(s):  
A. Glasse ◽  
D. Lee ◽  
P. Parr-Burman ◽  
D. Hayton ◽  
E. Mazy

2010 ◽  
Vol 6 (S276) ◽  
pp. 335-342 ◽  
Author(s):  
Mark Clampin

AbstractThe James Webb Space Telescope is a large aperture (6.5 meter), cryogenic space telescope with a suite of near and mid-infrared instruments covering the wavelength range of 0.6 ?m to 28 ?m. JWSTs primary science goal is to detect and characterize the first galaxies. It will also study the assembly of galaxies, star formation, and the formation of evolution of planetary systems. JWSTs instrument complement offers numerous capabilities to study the formation and evolution of exoplanets via direct imaging, high contrast coronagraphic imaging and photometric and spectroscopic observations of transiting exoplanets.


2014 ◽  
Vol 50 (2) ◽  
pp. 92-102
Author(s):  
Piyal Samara-Ratna ◽  
Jon Sykes ◽  
Chris Bicknell ◽  
John Pye ◽  
Niels Christian Jessen ◽  
...  

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