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    41. http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-STScI-000400.pdf
    ... It holds the object classification information including `unknown' (0), `cosmic ray' (1), `defect' (2), `galaxy' (3), `ghost' (4), `known object' (5), `star' (6), `star trail' (7), and `sky' (8). ...
    [ Текст ]  Ссылки http://www.stsci.edu/jwst/doc-archive/technical-reports/JWST-STScI-000400.pdf -- 620.7 Кб -- 05.02.2013
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    42. http://www.stsci.edu/hst/acs/documents/isrs/CTE_White_Paper_DELETE_DUPLICATE.pdf
    ... in$the$"charge$ trails"$that$follow$hot$pixels,$cosmic$rays,$and$bright$stars ... stars,$hotter$pixels,$or$ cosmic$rays$(which$typically$deposit$~103$ef)$will$still ...
    [ Текст ]  Ссылки http://www.stsci.edu/hst/acs/documents/isrs/CTE_White_Paper_DELETE_DUPLICATE.pdf -- 1757.7 Кб
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    43. http://www.stsci.edu/~kgordon/papers/PS_files/upper_sco_ob2.ps.gz
    ... The parallel linear streaks are trailed bright star images or scratches made as the film advanced. -- 5 -- ratio, FN =F S , was determined. ...
    [ Текст ]  Ссылки http://www.stsci.edu/~kgordon/papers/PS_files/upper_sco_ob2.ps.gz -- 842.6 Кб -- 23.04.2003
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    44. Pixel-Based CTI Corrections for STIS CCD Data
    ... The archive image shows significant trailing on stars and hot pixels, which is greatly reduced in the corrected image. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/stis/software/analyzing/scripts/pixel_based_CTI -- 20.9 Кб -- 11.04.2016
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    45. http://www.stsci.edu/spss/13056.status
    ... Colors of Giant Lya Nebulae 12679 Luminosity-Distance Standards from Gaia and HST 12756 X-raying the spectacular star-forming trail behind IC 3418 12803 Guard Darks 12861 Morphologies of the Most UV luminous Lyman Break Galaxies at z~3 12870 The mass and ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/spss/13056.status -- 19.2 Кб -- 19.02.2013
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    46. http://www.stsci.edu/~mutchler/documents/AJ_2006_Pluto_constraints.pdf
    ... combination removes artifacts, such as cosmic-ray events or star trails, that do not appear in same position on the plane of ... As a result, stars would appear as trails moving through the displayed region, and cosmic-ray events and bad pixels would ...
    [ Текст ]  Ссылки http://www.stsci.edu/~mutchler/documents/AJ_2006_Pluto_constraints.pdf -- 239.8 Кб -- 04.10.2006
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    47. Astronomy Outreach Images Workshop (ORIWORKS)
    ... 1:30pm . Timelapse and Art . Digital Star-trails and Nighttime Timelapse Animations . Peter Michaud . Kirk Pu'uohau-Pummill . Gemini Observatory . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/oriworks_dev/program.html -- 13.0 Кб -- 26.09.2003
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    48. Workshop Program Speakers
    ... 1:30pm . Timelapse and Art . Digital Star-trails and Nighttime Timelapse Animations . Peter Michaud . Kirk Pu'uohau-Pummill . Gemini Observatory . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/oriworks/program.html -- 23.9 Кб -- 10.04.2016
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    49. WFC3 Data Handbook
    ... The amplitude of the persistence for the brightest pixels in the diagonal trails of stars is about 0.1 electrons/sec The image is plotted on a linear scale from 0.7 to 0.9 electrons/sec . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/HST_overview/documents/datahandbook/hst/wfc3/documents/handbooks/currentDHB/Chapter8_persistence2.html -- 129.9 Кб -- 12.04.2016
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    50. http://www.stsci.edu/~mutchler/talks/Pluto_moons_poster.ppt.pdf
    ... show some residuals from the incomplete rejection of the artifacts evident in the individual "raw" images (Figure 1): star trails, cosmic rays, diffraction spikes, saturation and bleeding of overexposed Pluto and Charon, and the WFC interchip gap (where ...
    [ Текст ]  Ссылки http://www.stsci.edu/~mutchler/talks/Pluto_moons_poster.ppt.pdf -- 1932.8 Кб -- 19.12.2005
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