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    31. Data Quality Control at the Very Large Telescope
    ... The parameters presently supported by the QC0 application in place for UT1 include airmass, moon distance, fractional lunar illumination, and seeing, and correspond to the observation constraints available in the Phase II Preparation System. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/P2-17/ -- 14.4 Кб -- 11.10.2000
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    32. http://www.adass.org/adass/proceedings/adass94/mcdonaldk.ps
    ... the exciting early scientific results are the first complete EUV all­sky survey, the first EUV images of extended objects (e.g., the Moon, the Vela and Cygnus supernova remnants, and the Jupiter­Io plasma torus), and the first detection of helium on Mars ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass94/mcdonaldk.ps -- 65.9 Кб -- 13.06.1995
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    33. http://www.adass.org/adass/proceedings/adass02/reprints/O10-2.pdf
    ... Example 2: Locate the areas most frequently observed with an instrument in which the seeing is < 1 and the moon is below the horizon during the observation to produce very long exposures or perform time variation studies. ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass02/reprints/O10-2.pdf -- 137.7 Кб -- 11.03.2003
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    34. ADASS 2002 Conference Proceedings
    ... Example 2: Locate the areas most frequently observed with an instrument in which the seeing is and the moon is below the horizon during the observation to produce very long exposures or perform time variation studies. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass02/O10-2/ -- 16.3 Кб -- 12.03.2003
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    35. http://www.adass.org/adass/proceedings/adass03/reprints/P1-5.pdf
    ... Individual CCD exposures are adjusted according to moon phase to limit background contribution to the exposure. ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P1-5.pdf -- 76.2 Кб -- 27.08.2004
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    36. http://www.adass.org/adass/proceedings/adass03/reprints/P2-25.pdf
    ... Wide Field Imager) an estimate of the limiting magnitude given the overall sensitivity and parametrisation of the telescope/instrument/filter/detector and given the start time of the observation by which the sky brightness (Moon dependent) is evaluated ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P2-25.pdf -- 75.9 Кб -- 27.08.2004
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    37. http://www.adass.org/adass/proceedings/adass97/reprints/giulianom.pdf
    ... Constraint windows include sun avoidance, moon avoidance, user window constraints, phase constraints, roll constraints, guide star constraints, and time linkages between observations. ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass97/reprints/giulianom.pdf -- 80.5 Кб -- 14.04.1998
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    38. ADASS 2003 Conference Proceedings
    ... Individual CCD exposures are adjusted according to moon phase to limit background contribution to the exposure. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass03/P1-5/ -- 17.7 Кб -- 27.08.2004
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    39. ADASS 2003 Conference Proceedings
    ... Wide Field Imager) an estimate of the limiting magnitude given the overall sensitivity and parametrisation of the telescope/instrument/filter/detector and given the start time of the observation by which the sky brightness (Moon dependent) is evaluated ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass03/P2-25/ -- 16.1 Кб -- 27.08.2004
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    40. The NGST Mission Simulator
    ... The schedulability of the visits are also restricted by sun and moon avoidance constraints. ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/P1-17/ -- 16.1 Кб -- 09.10.2000
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