... magnitude M appearing on a given plate, we compute the luminosity function for the ... magnitude of objects is biased when measured near a plate edge, we calculate an ...
... magnitudes derived by DAOPHOT II, DASHA can automatically produce final color ... from instrumental magnitude lists produced by DAOPHOT II, to final color-magnitude ... can be filtered using magnitude vs.. magnitude error and magnitude vs. goodness-of ...
... magnitude M app earing on a given plate, we compute the luminosity function for the ... magnitude of ob jects is biased when measured near a plate edge, we calculate an ...
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Ссылки http://www.adass.org/adass/proceedings/adass96/reprints/smirnovo1.pdf -- 178.3 Кб -- 14.01.1998 Похожие документы
... magnitudes derived by DAOPHOT II, DASHA can automatically produce final color ... from instrumental magnitude lists produced by DAOPHOT II, to final colormagnitude ... can be filtered using magnitude vs.. magnitude error and magnitude vs. goodnessof ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/smirnovo1.ps -- 116.8 Кб -- 13.06.1995 Похожие документы
... 3 . 1 Recalibrating Aspect Camera Magnitude . 3 . 2 Recalibrating Spoiler Codes . ... use of AGASC, we recalibrated the estimated ACA magnitudes based on Chandra on-orbit ...
... We selected m B , because: ( i ) it yields good correlation with GSC magnitudes, ( ii ) it is more representative in RC3 than other magnitudes, and ( iii ) it is close to the system used in the stellar distribution. ...
... Coordinates, magnitudes, morphological data and proper motions are available for all ... object catalogues with user-specified magnitude range and output format (FITS, ASCII ...
... Coordinates, magnitudes, morphological data and proper motions are available for all ... 10 ) ob ject catalogues with userspecified magnitude range and output format (FITS ...
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Ссылки http://www.adass.org/adass/proceedings/adass00/reprints/P3-17.pdf -- 96.6 Кб -- 29.05.2001 Похожие документы