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    1. http://www.stsci.edu/jwst/instruments/miri/docarchive/miri-pocket-guide.pdf
    ... in nine (9) photometric bands from 5 to 28 µm, / ~ 5, with a field of view (FOV ) 74 ... sks (4QPMs) at 10.65, 11.4, & 15.5 µm (24'' x 24''), and a Lyot coronagraph at 23 µm ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/instruments/miri/docarchive/miri-pocket-guide.pdf -- 1576.4 Кб
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    2. http://www.stsci.edu/jwst/science/sodrm/highlightSpecProtoPlanetaryDisks.pdf
    ... Way Galaxy NIRSpec (R~2700/1-5 µm) can reach protoplanetary disks around Solar mass ... MIRI can obtain 5-28 µm R~2700 spectra of protoplanetary disks out to 7 kpc. ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/science/sodrm/highlightSpecProtoPlanetaryDisks.pdf -- 806.4 Кб -- 05.02.2013
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    3. http://www.stsci.edu/jwst/doc-archive/presentations/JWST-STScI-000438.pdf
    ... 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 ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/presentations/JWST-STScI-000438.pdf -- 451.9 Кб -- 05.02.2013
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    4. http://www.stsci.edu/jwst/doc-archive/presentations/DavidLafreniere.pdf
    ... 2010 1.5 Wavelength (µm) 2.0 2.5 Same model Transit spectroscopy possibilities Around a G dwarf Transit depth Jupiter/Neptune ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/presentations/DavidLafreniere.pdf -- 2750.6 Кб -- 05.02.2013
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    5. http://www.stsci.edu/jwst/instruments/nirspec/docarchive/NIRSpec-pocket-guide.pdf
    ... texp=105s 1 2 3 600 10 05s R=2700 S/N=10 texp=105 R=2700s Wavelength ( m) 3 4 5 Continuum ux F (nJy) v )00 10 05 00 s 4 5 Wavelength ( m) 0 1 2 Wavelength ( m) R=1000 S/N=10 texp=105s 3 R=2700 S/N=10 texp=105s 4 5 5x10 1 Wavelength ( m) 1500 10-18 4 5 1 1 ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/instruments/nirspec/docarchive/NIRSpec-pocket-guide.pdf -- 1443.3 Кб
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    6. http://www.stsci.edu/jwst/doc-archive/flyers/JWST-Asteroids-Comets.pdf
    ... phase masks (4QPMs) at 10.6 5, 11.4,and 15.5 µm ·Lyot coronagraph at 23 µm Low-Resolution Spectroscopy (LRS) ·5 to ~ 14 µm · l ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/flyers/JWST-Asteroids-Comets.pdf -- 959.5 Кб
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    7. http://www.stsci.edu/jwst/doc-archive/flyers/JWST-Proto-Planet.pdf
    ... Direct Imaging · nine photometric bands from 5 to 28 µm Coronagraphic Imaging · three four-quadrant phase masks (4QPMs) at 10.65, 11.4, & 15.5 µm, Lyot coronagraph at 23 µm Low-Resolution Spectroscopy (LRS) · 5-14 µm, l/Dl ~ 100 at 7.5 µm, 0.6'' x 5.5 ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/flyers/JWST-Proto-Planet.pdf -- 1649.5 Кб
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    8. http://www.stsci.edu/documents/dhb/web/c19_nicerror.fm1.html
    ... to a factor of ~3 at a wavelength of 2.2?m, and at 2.5 ?m the array is almost flat ... 2 , for a wavelength of 1.5 ?m. The figure shows that the variations are essentially ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/documents/dhb/web/c19_nicerror.fm1.html -- 10.0 Кб -- 17.11.1997
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    9. MIRI At A Glance
    ... Document Archive . Glossary . Meetings . ? = 5 - 28.3 m . 1.25' x 1.88' field of view . ... 1.25' x 1.88' field of view . Low resolution spectrograph, R~100, 5-10 m . ... Blackened Blank . N/A . For Darks . ? = 5 - 27 m (goal is 28.3 m) . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/jwst/instruments/miri/miri-glance -- 20.2 Кб -- 10.04.2016
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    10. http://www.stsci.edu/~kgordon/papers/PS_files/spitzer_newviews_m101.pdf
    ... at 3.6, 4.5, 5.8, 8.0 µm and with the Multiband Imaging Photometry for Spitzer (MIPS ... and the mosaicking was done 5.8 µm images suffered from poor dark subtraction be ...
    [ Текст ]  Ссылки http://www.stsci.edu/~kgordon/papers/PS_files/spitzer_newviews_m101.pdf -- 352.9 Кб -- 01.03.2005
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