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    1. Figure 65
    ... Fig. 65 M = 10 6 M . M low = 1 M . Download here . Download here . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/starburst99/figs/fig65.html -- 2.6 Кб -- 21.08.1998
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    2. http://www.stsci.edu/jwst/instruments/miri/docarchive/miri-pocket-guide.pdf
    ... e (3) four- quadrant pha se ma sks (4QPMs) at 10.65, 11.4, & 15.5 µm (24'' x 24''), and a Lyot coronagraph at 23 µm (30'' x 30 ... MRS Continuum Sensitivit y 4QPM's! (24" x 24")! 10.65 µm! 11.4 µm! 15.5 µm! Lyot! (30" x 30")! 23 µm! Imager! (74" x 113 ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/instruments/miri/docarchive/miri-pocket-guide.pdf -- 1576.4 Кб
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    3. http://www.stsci.edu/institute/conference/acs_hls/clampin.pdf
    ... A-B) 98242MABR10-02 (C-D) 15 µ m x 15 µ m 15 µ m x 15 µ m 2048 x 4096 2048 x 4096 77000 e77000 e6.2 e-/pix/ hr m m m m m m m m 65% 68% 74% 74% 62% 37% 24% 13% 4. 9 e4.9 e7.0 e-/pix/ hr 66% 70% 76% 75% 60% 36% 23% 12% 5.3 e5.0 eWFPC2 STIS WFC#1 WFC#2 HRC ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/acs_hls/clampin.pdf -- 1794.7 Кб -- 28.03.2006
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    4. http://www.stsci.edu/hst/observatory/documents/isrs/isr_calscs_009.pdf
    ... agrees with NL84 spectrum to 2-3 in the 0.45 to 0.65 m range and has 2 to 4 more ux than NL84 spectrum in the entire 0.65 to 0 ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/observatory/documents/isrs/isr_calscs_009.pdf -- 230.6 Кб -- 14.11.2003
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    5. http://www.stsci.edu/hst/wfc3/documents/ISRs/2002/WFC3-2002-13.pdf
    ... WFC3 IR has a long-wavelength cutoff at ~1.65 µm; since for sufficiently large limb angle (>50, see Giavalisco, Sahu, & Bohlin ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs/2002/WFC3-2002-13.pdf -- 63.7 Кб -- 25.09.2008
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    6. http://www.stsci.edu/~INS/2010CalWorkshop/chayer.pdf
    ... As for the 2MASS p oint source catalog, it contains 0.47 billion ob jects over the entire sky in the J (1.25 µm), H (1.65 µm), and KS (2.16 µm) band passes and is complete down to J 16. ...
    [ Текст ]  Ссылки http://www.stsci.edu/~INS/2010CalWorkshop/chayer.pdf -- 267.4 Кб -- 23.04.2012
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    7. GigaCAM
    ... With back illumination, the QE at 1 m m is 65% (at T=150 K). ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/space_detectors/giga.htm -- 41.3 Кб -- 30.08.2001
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    8. http://www.stsci.edu/hst/nicmos/documents/isrs/isr_99_007.pdf
    ... Sosey at wavelengths of 1.10, 1.60, and 1.65 µm. The PSFs were not subsampled and were generated using the default weighting ... Encircled Energies for the Synthetic Dataset Wavelength (µm) 1.10 1.60 1.65 1.10 1.60 1.65 Radius (Pixels) 3 3 3 6 6 6 ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/nicmos/documents/isrs/isr_99_007.pdf -- 224.2 Кб -- 12.02.2002
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    9. http://www.stsci.edu/hst/nicmos/documents/isrs/isr_98_014.pdf
    ... The ground-based IR background (filled triangles) was measured from J (1.25 µm), H (1.65 µm), and Ks (2.14 µm) observations obtained at the Las Campanas 2.5-m telescope with a NICMOS3 array, during dry weather. ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/nicmos/documents/isrs/isr_98_014.pdf -- 110.2 Кб -- 12.02.2002
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    10. FGS Transfer Mode Reference Targets
    ... HD 59149 . 6.70 . 1.28 . 7 h 29 m 30.65 s . +19 o 38' 00.00" . HD 233877 . 9.70 . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/fgs/dataanalysis/reffiles/tmreference.html_not_used -- 41.3 Кб -- 11.04.2016
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