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    • [ В начало ] Пред. | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | След.

    91. http://www.stsci.edu/hst/nicmos/documents/isrs/isr_98_013.pdf
    ... sources clump around 40% of the flux in the peak pixel, while a "tail" of sources with much more of the flux (up to 60%) in the ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/nicmos/documents/isrs/isr_98_013.pdf -- 13.2 Кб -- 12.02.2002
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    92. http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2007-26.pdf
    ... the dark current rate because of the bias introduced by the hot pixel tail ... To avoid this, the hot pixel tail is sometimes reduced with sigma-clipping. ... a log-normal Gaussian or with a Gaussian and an exponential drop-off for the tail ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2007-26.pdf -- 252.7 Кб -- 28.11.2007
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    93. http://www.stsci.edu/hst/HST_overview/documents/multidrizzle/ch65.html
    ... and artifacts (e.g. stars and cosmic rays) may have prominent comet-like tails of deferred charge in the anti-readout direction ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/HST_overview/documents/multidrizzle/ch65.html -- 17.4 Кб -- 05.02.2013
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    94. http://www.stsci.edu/hst/HST_overview/documents/calworkshop/workshop2005/papers/kimble.pdf
    ... produced for WFC3 exhibit higher dark current tails than seen in FPA64 (Figure 11 ... QE curves shows systematically larger dark current tails than the lower QE group ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/HST_overview/documents/calworkshop/workshop2005/papers/kimble.pdf -- 613.3 Кб -- 04.04.2006
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    95. http://www.stsci.edu/ftp/observing/status_reports/old_reports_00/hst_status_08_23_00
    ... Light from Old Stellar Populations: A Census of UV Bright Stars in `Blue Tail' Globular Clusters) The WF/PC-2 was used to make ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_00/hst_status_08_23_00 -- 8.8 Кб -- 23.08.2000
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    96. http://www.stsci.edu/hst/wfc3/documents/ISRs/2001/WFC3-2001-05.pdf
    ... Cosmic Ray Tails-WFPC2 and STIS The Cosmic Ray Tails from dark frames were analyzed ... tail length is an indication of the release timescale for the traps since the tail ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs/2001/WFC3-2001-05.pdf -- 683.8 Кб -- 25.09.2008
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    97. http://www.stsci.edu/spst/UnixTransition/doc/check_69.py
    ... tail) = os.path.split(rmsfile) # If there is an extension present in tail, then strip it out, when # constructing rptfile. posdot = string.find(tail,".") if (posdot != -1): rptfile = tail[:posdot] + "_69.rpt" else: rptfile = tail + "_69.rpt" else: # Get ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/spst/UnixTransition/doc/check_69.py -- 24.8 Кб -- 28.02.2014
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    98. http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2008-02.pdf
    ... say) with the cold detector, the hot pixel tail is at a very low level with respect ... temperatures, the level needs to be increased to remain above the hot pixel tail ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfc3/documents/ISRs/WFC3-2008-02.pdf -- 96.7 Кб -- 31.01.2008
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    99. http://www.stsci.edu/ftp/observing/status_reports/old_reports_00/hst_status_08_24_00
    ... Light from Old Stellar Populations: A Census of UV Bright Stars in `Blue Tail' Globular Clusters) The WF/PC-2 was used to make ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_00/hst_status_08_24_00 -- 9.0 Кб -- 24.08.2000
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    100. http://www.stsci.edu/institute/stuc/apr07-presentations/WFPC2Update.pdf
    ... light reduces loss (pre-fills traps) Tails are seen on bright pixels as charge ... Bright Target Pixel 4 Example of "tail" on 310 DN target caused by CTE effect. ... Tail contains 9% of the total counts. ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/stuc/apr07-presentations/WFPC2Update.pdf -- 1305.9 Кб -- 17.04.2007
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