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    81. http://www.stsci.edu/documents/dhb/web/c20_nicdataanal.fm2.html
    ... Given the multitude of units and systems that have been used for infrared (IR) photometry (magnitudes, Jy, W m -2 ?m -1 , erg sec -1 cm -2 ?m -1 , etc.) and given the lack of a standard for ground-based IR filters, NICMOS has adopted the IRAS approach ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/documents/dhb/web/c20_nicdataanal.fm2.html -- 30.4 Кб -- 17.11.1997
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    82. STScI Preprint #1293
    ... The temporal evolution of the first and second overtones of CO at 2.29 m (2-0 bandhead) and 1.62 m (6-3 bandhead) and of the (U-B), (B-V) and (J-K) colors are investigated. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1293/prep1293.html -- 5.2 Кб -- 23.05.2000
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    83. The 24 Micron Source Counts in Deep Spitzer Space Telescope Surveys
    ... on the 24 ЮМm background intensity of 1.9+/-0.6 nW m-2 sr-1 of which the majority (~60%) stems from sources fainter than 0.4 ... sources below 60 ЮМJy contribute 0.8+0.9-0.4 nW m-2 sr-1 to the background, which provides an estimate of the total 24 ЮМm ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2004ApJS..154...70P.html -- 4.8 Кб -- 21.01.2016
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    84. http://www.stsci.edu/jwst/doc-archive/presentations/JWST-STScI-000439.pdf
    ... 02-JWST-0001 - 3 Observatory Design Requirements Requirement Value Estimated Performance 29.4 m 8 2% 2 Aperture >25 m2 collecting area Encircled Energy >75% for 150 mas radius at 1 µm PSF Stability <2% RMS variation about mean over 24 hours at 150 mas ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/presentations/JWST-STScI-000439.pdf -- 895.8 Кб -- 05.02.2013
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    85. http://www.stsci.edu/jwst/doc-archive/white-papers/JWST_scientific_cap.pdf
    ... the telescope will be diffraction limited at 2 m, defined as having a Strehl ratio ... resolution is 68 milli-arcsec at 2 m. The fine guidance sensor provides a >95 ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/white-papers/JWST_scientific_cap.pdf -- 1022.2 Кб -- 05.02.2013
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    86. http://www.stsci.edu/ftp/documents/fos-handbook/table_121.ps
    ... 6.83x10 30 F l DlE l T l l ­­­­­­­­­­­­­­­­­­­­­­­­­­­­­­­ F n F n 5556 , ­­­­­­­­­­­­­­­­­­­­­­ m 5556 , 2.38x10 11 F n F n 5556 , ­­­­­­­­­­­­­­­­­­­­­­ DlE l T l l ­­­­­­­­­­­­­­­­­­­­­­­­ 10 0.4m 5556 -- a m 5556 , 2.38x10 11 l 5556 ­­­­­­­­­­­­­ Х Ь ...
    [ Текст ]  Ссылки http://www.stsci.edu/ftp/documents/fos-handbook/table_121.ps -- 60.2 Кб -- 16.06.1994
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    87. http://www.stsci.edu/instrument-news/handbooks/nicmos/c06_exptime.doc5.html
    ... from the ground to have a strength of 10 -13 W/m 2 and negligible continuum ... we determine that the surface brightness in the line is 1.5 x 10 -14 W/m 2 /arcsec 2 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instrument-news/handbooks/nicmos/c06_exptime.doc5.html -- 20.5 Кб -- 07.08.1997
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    88. http://www.stsci.edu/hst/observatory/documents/isrs/otaisr2001-01.pdf
    ... As can be seen, during SMOV3A, a focus adjustment was made (2000.009, +4.2µm). ... m) see figure 2 4 9 Jan 00 (+4.2µm) Instrument Science Report OTA 2001-01 Ultimately ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/observatory/documents/isrs/otaisr2001-01.pdf -- 860.7 Кб -- 14.11.2003
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    89. JWST Science Corner
    ... throughput of 15%, and utilizes NIRISS?s F277W (2.77 ?m), F380M (3.8 ?m), F430M (4.3 ... by non-redundant masking on future 2.4 m and 16 m space telescopes working at long ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/jwst/jwst-science-corner/paper-abstracts-agn -- 20.1 Кб -- 10.04.2016
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    90. http://www.stsci.edu/hst/nicmos/documents/isrs/isr95_006.pdf
    ... variations (a factor of four across the array at 1.2µm), and their substantial variation with wavelength (from a factor of ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/nicmos/documents/isrs/isr95_006.pdf -- 351.5 Кб -- 12.02.2002
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