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    91. http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_04_10_96
    ... being run today, HST operations = personnel moved to the SAMS backup facility at 101/0600Z. 3.0 SIGNIFICANT FORTHCOMING EVENTS: GSFC Internal Simulation #3 (EVA #3 - DIU/SSR/SADE) will be = conducted from approximately 8:00 a.m. to 8:00 p.m today ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_96/hst_status_04_10_96 -- 3.6 Кб -- 10.04.1996
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    92. http://www.stsci.edu/science/starburst/Preprints/iau212.pdf
    ... Left: Ratio of [Ne III] 15.6 µm over [Ne II] 12.8 µm vs. ... The [Ne I I I] 15.6 µm and [Ne I I] 12.8 µm lines are particularly useful. ... IV] 25.9 µm to [Ne I I] 12.8 µm line flux ratio versus the strength of the PAH bands ...
    [ Текст ]  Ссылки http://www.stsci.edu/science/starburst/Preprints/iau212.pdf -- 449.5 Кб -- 10.07.2002
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    93. http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-STScI-001375.pdf
    ... 0. 824 536 575187 11. 50 41178. 0 76. 8m + F212N 4µ m + F444W 4µ m + F410M 1 ... 0.164 0.041 0.010 Fsat [Jy/ arcsec2] 2 µm 0.54 2.14 8.56 34.25 136.99 547.96 4 µm 0 ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-STScI-001375.pdf -- 652.6 Кб -- 05.02.2013
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    94. http://www.stsci.edu/ftp/observing/status_reports/old_reports_01/hst_status_05_23_01
    ... FORTHCOMING EVENTS: GSFC Internal Simulation #8 (EVA-1 -- -V2 SA wing), a three-day exercise, will begin this morning at 8:00 a.m. Today's session will conclude at approximately 8:00 p.m. Continuation of normal science observations and calibrations ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_01/hst_status_05_23_01 -- 5.7 Кб -- 23.05.2001
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    95. http://www.stsci.edu/~marel/decadal/sc/302.pdf
    ... Current 8­10 m telescopes can obtain spectra with adequate signal-to-noise to ... and Leo T), spectroscopy with current 8­10 m telescopes is practical for individual ...
    [ Текст ]  Ссылки http://www.stsci.edu/~marel/decadal/sc/302.pdf -- 351.1 Кб -- 19.02.2009
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    96. http://www.stsci.edu/hst/nicmos/documents/isrs/isr_2005_002.pdf
    ... in their overlap region at 0.8-1.0µm, the ratios of the STIS and NICMOS fluxes for ... and the STIS G750L overlap from 0.8 to 1µm. However, there is a disagreement between ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/nicmos/documents/isrs/isr_2005_002.pdf -- 1043.7 Кб -- 19.11.2007
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    97. http://www.stsci.edu/~marel/abstracts/psdir/n7052_5.ps
    ... 5 \Theta 10 8 M fi . ... 5 \Theta 10 8 M fi ; Dressel, Bania & O'Connell 1982). ... nuclear black hole : MBH = 0, 1:5 \Theta 10 8 M fi , 5 \Theta 10 8 M fi and 1:5 ...
    [ Текст ]  Ссылки http://www.stsci.edu/~marel/abstracts/psdir/n7052_5.ps -- 1234.1 Кб -- 26.04.1997
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    98. STScI Preprint #1322
    ... Kune 6 , Du lia F. de Mello, 7 Daniel Devost, 8 Timothy M. Heckman 9 Starburst99 is a comprehensive set of model predictions ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1322/prep1322.html -- 6.0 Кб -- 21.12.2005
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    99. http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-STScI-000395.pdf
    ... NGST's) mid-infrared ( = 5 - 2 8 µ m) background under the assumption that a small ... Strictly speaking, NGST Monograph 3 considered an 8-m OTE. ... emission becomes dominanant at 12.4 m with a flux at the detector 297.8 e s pixel ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-STScI-000395.pdf -- 2334.5 Кб -- 05.02.2013
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    100. http://www.stsci.edu/institute/conference/hsl/Nelson.PDF
    ... their study Hubble Legacy 5apr02 jen 8 Scientific Potential · Seeing limited observations ­ 0.3 - 1.0 µm ­ Scale 2.18 mm/arc ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/hsl/Nelson.PDF -- 2035.8 Кб -- 10.04.2006
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