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    • 1 | 2 | След.

    1. Scatter light Measurements on APO 3
    ... to noise, lack of intrinsic moon glow gradients, and least number of star trails ... The 3 peaks below row 400 are from star trails in this image. ... 50 columns were averaged here owing to the large number of star trails in this image ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/users/morgan/APO/Scattered.light.measurements/The%20Interim%20Report.htm -- 127.5 Кб -- 15.03.2004
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    2. http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/Echelle/PDF/echelle_quickstart.pdf
    ... For sufficiently bright sources (usually mV < 10), the sampling of the star on the slit can be improved by trailing the star across the slit during the exposure. ...
    [ Текст ]  Ссылки http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/Echelle/PDF/echelle_quickstart.pdf -- 297.4 Кб -- 22.05.2005
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    3. TUI:Scripts:Built In Scripts:Telescope:Pointing Data
    ... star cannot be measured, continue on to the next star, but pause at the very end if ... Stars : add all stars from Missing Stars (except those in Stars to Skip ) to Stars ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/35m_operations/TUI/Scripts/BuiltInScripts/PointingData.html -- 7.6 Кб -- 05.09.2014
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    4. TUI:Scripts:Built In Scripts:Echelle:Trail
    ... As Don York explained: trailing is used with the echelle to distribute charge over the CCD, especially for bright star work. ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/35m_operations/TUI/Scripts/BuiltInScripts/EchelleTrail.html -- 3.1 Кб -- 05.09.2014
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    5. Hipparcos Tycho catalog
    ... The ACT contains 93% of the Tycho catalog stars. ... The lower the surface density of these stars on the sky, the more stringent the ... Consequently, it is useful to know the surface density distribution of Tycho stars. ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/SDSS/eng.papers/19970901_TychoDensity/19970901.html -- 6.7 Кб -- 19.05.1998
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    6. http://www.apo.nmsu.edu/arc35m/Instruments/ARCES/images/arcechellspie.pdf
    ... a quadrant balance of the wings of the image of the guide star; and to auto trail along the long dimensions of the aperture ...
    [ Текст ]  Ссылки http://www.apo.nmsu.edu/arc35m/Instruments/ARCES/images/arcechellspie.pdf -- 748.4 Кб -- 29.06.2010
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    7. Instrument Data Fitting
    ... to a fairly bright (for the instrument) isolated star high in the sky and near the ... Leading and trailing lines that do not begin with digits will be ignored. boresight ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/TCC/InstDataFit.html -- 12.6 Кб -- 10.09.2015
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    8. Focus sweep data
    ... Four images were obtained from each focus sweep; 1) CCD g1, at the trailing corner of the CCD array; 2) CCD g3, near the middle of the trailing edge; 3) CCD u1, at the edge of the central row of CCDs; 4) CCD u3, near the center of the CCD array. ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/SDSS/mirror_report/node5.html -- 15.2 Кб -- 24.11.1999
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    9. TCC Commands
    ... a position reference star near the target, and slew to center the reference star in ... star nearest the position specified by the TRACK command (or the current object if ...
    [ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/TCC/Commands.html -- 76.3 Кб -- 31.03.2015
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    10. http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/Echelle/PDF/ARCES_data_guide.pdf
    ... Use a standard star to define approximate aperture locations and traces, then extract desired orders from the standard star using noao.imred.echelle.apall. ...
    [ Текст ]  Ссылки http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/Echelle/PDF/ARCES_data_guide.pdf -- 410.4 Кб -- 25.09.2000
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