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    101. STScI Preprint #????
    ... the many interesting results obtained from UV observations of SN 1987A, we focus on two aspects: (1) the detection and the study of a UV echo from SN 1987A, and (2) the determination of the distance to SN 1987A based on UV and optical observations of SN ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1319/prep1319.html -- 5.5 Кб -- 14.07.2000
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    102. STScI Preprint #1294
    ... UV Diagnostics of the Interaction between Starburst Galaxies and the Intergalactic ... these problems rely heavily on access to the rest-frame ultraviolet (UV) spectrum ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/science/preprints/prep1294/prep1294.html -- 4.4 Кб -- 23.05.2000
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    103. http://www.stsci.edu/ftp/observing/status_reports/old_reports_00/hst_status_11_16_00
    ... UV Imaging Survey of IR-Bright Star- Forming Galaxies) The Space Telescope Imaging Spectrograph (MA1) was used to carry out a UV ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_00/hst_status_11_16_00 -- 6.4 Кб -- 16.11.2000
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    104. http://www.stsci.edu/ftp/instrument_news/FOC/Foc_docs/Cycle6cal_table.ps
    ... UV Throughput Monitoring 3% monitor UV throughput 6894 Aperture Location Monitoring 0.2'' monitor pointing stability 6895 PSF Monitoring 2µ monitor image quality Geometric Distortion Monitoring monitor stability of geometric distortion Special Calibration ...
    [ Текст ]  Ссылки http://www.stsci.edu/ftp/instrument_news/FOC/Foc_docs/Cycle6cal_table.ps -- 54.3 Кб -- 10.05.1996
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    105. Introduction
    ... The broad-band filter series extends into the far UV. There is a Str mgren series. ... A Wood's filter is available for far-UV imaging without a red leak. ... s filter may be crossed with another UV filter to provide a solar blind passband ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instrument-news/handbooks/wfpc2/W2_23.html -- 8.7 Кб -- 24.07.1996
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    106. http://www.stsci.edu/ftp/science/hdf/hdfsouth_old/project/stisflow.ps
    ... STIS Observations UV Spectroscopy 40 Orbits Echelle ­ 1150­3100е ­ 6­10 km/s resolution ­ 0.1­0.2е EW limit (5 s) 10 Orbits Low­ Resolution ­ 1150­3100е ­ 250­400 km/s resolution ­ 0.5­0.7е EW limit UV Imaging 5 Orbits FUV ­ 1500­1700е ­ AB=27.0 mag limit ...
    [ Текст ]  Ссылки http://www.stsci.edu/ftp/science/hdf/hdfsouth_old/project/stisflow.ps -- 57.9 Кб -- 01.07.1998
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    107. CALOBS
    ... CALOBS contains several versions of the ultraviolet (UV) and optical spectra of the fundamental flux standards used for HST ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instruments/observatory/cdbs/calobs.html -- 5.7 Кб -- 02.07.2001
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    108. The CO Abundance on Neptune from its UV Reflection Spectrum
    ... Electronic Editor: H. Payne . The CO Abundance on Neptune from its UV Reflection Spectrum . Abstract: . Introduction . ... scattering is found to have a dominant influence on the UV albedo of Neptune in that spectral range, whereas haze particles ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/shst2/courtinr.html -- 16.3 Кб -- 15.06.2005
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    109. Which Instrument to Use: WFPC2, FOC, NICMOS, or STIS?
    ... of HST instruments with imaging capability in the UV to near-IR spectral range ... Higher throughput at l<4500 . Less impacted by far-UV contaminants. ... Much higher UV throughput. True solar blind imaging in UV due to MAMA detectors. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instrument-news/handbooks/wfpc2/W2_4.html -- 7.6 Кб -- 24.07.1996
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    110. The Previous vs. Current Generation: WF/PC-1 vs. WFPC2
    ... decontaminations, since high temperatures would remove the UV flood, which in turn severely limited UV science capabilities ... This transmitted solar UV light into the camera to provide a UV flood capability. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instrument-news/handbooks/wfpc2/W2_6.html -- 8.7 Кб -- 24.07.1996
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