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    41. http://www.stsci.edu/~mutchler/talks/Calib_Workshop_2005.pdf
    ... trending) · Flag 32 redefined as "hot pixel CTE tails" (just the first trailing pixel for now) in superdark DQ · Flag 64 redefined as "warm pixels" between 0.02 and 0.08 e/sec (also gets more of the CTE tails) in superdark DQ · New flags provide optional ...
    [ Текст ]  Ссылки http://www.stsci.edu/~mutchler/talks/Calib_Workshop_2005.pdf -- 347.9 Кб -- 24.10.2005
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    42. http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_03_25_99
    ... the tidal tail of galactic merger NGC-3256W. By modeling these systems with N-body hydrodynamic codes, can we identify the physical circumstances and formation histories which can produce tidal dwarfs, star clusters, and other structures in tidal tails ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_03_25_99 -- 6.9 Кб -- 25.03.1999
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    43. http://www.stsci.edu/smov/SMOV4%20WEB%20PAGE%20OCT2007/smov4notes/NICMOS_SMOV_Report_20091007.pdf
    ... NIC3 shows a marked increase in the high current tail, indicating an increase in the low S/N structure 6 Recent Results NIC1 75K 76K 77K 15.8% 24.2% 29.4% Quantifying the warm dark current tail: Fraction of pixels above a dark current level (total ...
    [ Текст ]  Ссылки http://www.stsci.edu/smov/SMOV4%20WEB%20PAGE%20OCT2007/smov4notes/NICMOS_SMOV_Report_20091007.pdf -- 1256.0 Кб -- 08.10.2009
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    44. http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_11_19_98
    ... 7466 (From Globular Clusters to Tidal Dwarfs: Structure Formation in Tidal Tails ... of the globular clusters (et al.) within the tidal tail of galactic merger NGC-7252 ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_98/hst_status_11_19_98 -- 6.7 Кб -- 19.11.1998
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    45. Photometric Anomalies: CTE and Long vs. Short
    ... 4.18 , no significant tail is apparent at low Y. But at high Y an exponentially declining tail is readily apparent with an e ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instruments/wfpc2/Wfpc2_hand2/ch4_ccd13.html -- 32.4 Кб -- 29.08.2000
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    46. http://www.stsci.edu/hst/wfpc2/documents/isr/wfpc2_isr0501.pdf
    ... tail, we rejected any hot pixels where a pixel in the tail exceeded some threshold.2 ... tail has an additional faint component with a very slow decay (lower panel in Figure ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/wfpc2/documents/isr/wfpc2_isr0501.pdf -- 248.8 Кб -- 05.02.2013
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    47. Position Dependance of Linearity Beyond Saturation and Serial Transfer
    ... direction that take the form of long tails emanating from the saturated pixels ... central pixel shows a strong serial tail that continues through the serial overscan ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/cos/documents/newsletters/cos_stis_newsletters/full_stories/2013_06/CCD_linearity -- 24.2 Кб -- 12.04.2016
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    48. http://www.stsci.edu/institute/stuc/apr07-presentations/WFC3Update.pdf
    ... FPA 129, substrate removed, new BCS, significant dark tail) ­ ­ ­ ­ ­ Performance significantly exceeds FPA 64 even ignoring ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/stuc/apr07-presentations/WFC3Update.pdf -- 990.6 Кб -- 17.04.2007
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    49. Photometric Anomalies: CTE and Long vs. Short
    ... 4.18 , no significant tail is apparent at low Y. But at high Y an exponentially declining tail is readily apparent with an e ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/instruments/wfpc2/Wfpc2_hand4/ch4_ccd13.html -- 39.9 Кб -- 04.09.2001
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    50. Examples of Target List Blocks
    ... proposer wants to perform spectroscopy in the tail of comet Halley near the time of ... 3 . Name: . COMET-HALLEY-TAIL . Description: . OFFSET COMET HALLEY . Level_1: . ... SIZE = 1 . Comments: . 30 arcsec into tail of Halley during Giotto encounter. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/documents/p2pi/HTMLjavahelp21/ch04_targ_ss10.html -- 73.0 Кб -- 24.05.2013
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