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    • [ В начало ] Пред. | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | 17 | 18 | След.

    121. http://www.stsci.edu/hst/wfc3/documents/ISRs/2002/WFC3-2002-02.pdf
    ... average zodiacal background of 0.17 MJy/sr at 1.2 µm and 0.14 MJy/sr at 1.6 µm. The zodiacal light model presented in the NICMOS Handbook (v2 1997) supposedly providing mean values for an inclination of 45 degrees over the ecliptic, was used to verify 2 ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs/2002/WFC3-2002-02.pdf -- 54.2 Кб -- 25.09.2008
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    122. http://www.stsci.edu/smov/SMOV4%20WEB%20PAGE%20OCT2007/SMOV4%20Activity%20Summaries/WFC3.pdf
    ... Background light, as measured for each W&M filter from external images of a single field of medium zodiacal light level, will be compared to those anticipated from known sources (e.g. Zodiacal light) and WFC3 throughput (cf. ...
    [ Текст ]  Ссылки http://www.stsci.edu/smov/SMOV4%20WEB%20PAGE%20OCT2007/SMOV4%20Activity%20Summaries/WFC3.pdf -- 128.9 Кб -- 18.03.2009
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    123. http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_10_23_98
    ... 1.7 Completed NIC/2 7441 (A Search for Zodiacal Dust around Bright Nearby Stars) The Near Infrared Camera (Camera Two) was used to make observations of the zodiacal lights around the bright nearby star Sirius. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_10_23_98 -- 11.7 Кб -- 23.10.1998
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    124. http://www.stsci.edu/jwst/science/Solar-System-Science-FAQs-20121012.pdf
    ... JWST sensitivity will be limited by the zodiacal light background shortward of ~13 microns. ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/science/Solar-System-Science-FAQs-20121012.pdf -- 57.8 Кб -- 04.02.2013
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    125. Dark Current Measurements on a State of the Art Near
    ... choice of this cutoff wavelength is driven by the desire to be limited by the background contribution from the sky (zodiacal light) and the thermal emission of the telescope optics, given the anticipated detector operating temperature of 150 K. The basic ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/space_detectors/workshop2.htm -- 18.5 Кб -- 29.08.2001
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    126. http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_10_15_98
    ... 1.3 Completed Two Sets of NIC/2 7441 (A Search for Zodiacal Dust around Bright Nearby Stars) The Near Infrared Camera (Camera Two) was used to make observations of the zodiacal lights around the bright nearby star Altair. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_10_15_98 -- 9.5 Кб -- 15.10.1998
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    127. http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_10_21_98
    ... 1.10 Completed Two Sets of NIC/2 7441 (A Search for Zodiacal Dust around Bright Nearby Stars) The Near Infrared Camera (Camera Two) was used to make observations of the zodiacal lights around the bright nearby star Sirius. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_10_21_98 -- 9.6 Кб -- 21.10.1998
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    128. http://www.stsci.edu/ftp/stsci/newsletters/1999/stsci.news.1.99.pdf
    ... 5 Detector signal (electrons/pixel/sec) 1E+3 Zodiacal light 1E+1 1E­1 Dust scattered ... are needed for the observatory to be zodiacal-light-limited up to about 30 microns ...
    [ Текст ]  Ссылки http://www.stsci.edu/ftp/stsci/newsletters/1999/stsci.news.1.99.pdf -- 919.3 Кб -- 23.03.1999
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    129. http://www.stsci.edu/stsci/meetings/space_detectors/pdf/workshop2.pdf
    ... choice of this cutoff wavelength is driven by the desire to be limited by the background contribution from the sky (zodiacal light) and the thermal emission of the telescope optics, given the anticipated detector operating temperature of 150 K. The basic ...
    [ Текст ]  Ссылки http://www.stsci.edu/stsci/meetings/space_detectors/pdf/workshop2.pdf -- 127.1 Кб -- 22.08.2001
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    130. WFC3 Instrument Handbook
    ... These sources include zodiacal light, detector dark current, and stray light from both Earth and bright targets in the field of view. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/acs/hst/wfc3/documents/handbooks/currentIHB/c04_phaseI3.html -- 23.1 Кб -- 12.04.2016
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