... by ESA NASA provides focal planes, signal chain Consortium provides optical bench assembly · Functional capabilities include Imaging · =5-27 µm wavelength range · Diffraction limited imaging with 0.1" pixels · ~2 square arcmin field of view · Low ...
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Ссылки http://www.stsci.edu/jwst/doc-archive/presentations/JWST-STScI-000438.pdf -- 451.9 Кб -- 05.02.2013 Похожие документы
... t=1,000 s, 500 s, 250 s, and 125 s exposures using a 27 µm pixel pitch array ... The effect is most pronounced in 27 µm pitch InSb arrays at exposure times shorter ... see Barth & Isaac 1999), and the pixel pitch is 27 µm, one would expect 3.6% of the ...
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Ссылки http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-STScI-000387.pdf -- 1155.9 Кб -- 05.02.2013 Похожие документы
... SMOV Morning Meeting P o in tin g C o n tro l S y s te mM ay 27, 2009 May 27, 2009 P. 1 P C S P e rfo rm a n c e · Evaluation of vehicle jitter continues - Investigation closing in on G3 - 16.5 Hz frequency appears to be cause of increased jitter » 6 m a ...
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Ссылки http://www.stsci.edu/smov/SMOV4%20WEB%20PAGE%20OCT2007/smov4notes/SMOV_PCS.pdf -- 453.9 Кб -- 03.06.2009 Похожие документы
... N/A . For Darks . ? = 5 - 27m (goal is 28.3 m) . Integral field spectroscopy, 3.5" x 3.5" FOV (or more) . R ~ 3000-1000 from ? ... Integral field spectroscopy, 3.5" x 3.5" FOV (or more) . R ~ 3000-1000 from ? = 5- 27m . Channel . Wavelength . m . ...
... MIRI is a very flexible instrument, offering 5µm < < 27µm imaging, 5µm < < 14µm sp ectroscopy with R 100, and 5µm < < 27µm integral field unit sp ectroscopy with R 3000. ...
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Ссылки http://www.stsci.edu/hst/HST_overview/documents/calworkshop/workshop2005/papers/jer_proc.pdf -- 81.5 Кб -- 04.04.2006 Похожие документы
... 2007). Spectra are scaled to the peak flux at 1.27m. Fig. 2.- ... are scaled to the peak flux at 1.27m. halo (see, e.g., the discussion of kinematics ... 400 and scaled to the peak flux at 1.27m. 10 m. The effect is not as important in ...