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    41. Automated Spectral Classification Using Neural Networks
    ... IUE low-dispersion spectra of normal stars with spectral types ranging from O3 to G5 ... IUE Low-Dispersion Reference Atlas of Normal Stars (Heck et al. 1983), covering the ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass97/vieirae.html -- 9.9 Кб -- 15.05.1998
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    42. http://www.adass.org/adass/proceedings/adass96/reprints/smirnovo1.pdf
    ... H. E. Payne, eds. Refining the Guide Star Catalog: Plate Evaluations Oleg M. Smirnov ... and prop erties of plates digitized during creation of the Guide Star Catalog (GSC ... 1593 plates and by including bright stars from the HIPPARCOS INCA database ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass96/reprints/smirnovo1.pdf -- 178.3 Кб -- 14.01.1998
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    43. http://www.adass.org/adass/proceedings/adass96/reprints/karovska1.pdf
    ... Star/Fid Light Solutions: Calculate offset b etween fiducial light solutions and ... p oorlyfitting PSFs and find sp oiler stars in star and fiducial light images ... Sp oilers are faint stars in the vicinity of guide stars or fiducial lights). ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass96/reprints/karovska1.pdf -- 130.7 Кб -- 14.01.1998
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    44. http://www.adass.org/adass/proceedings/adass03/reprints/P2-36.pdf
    ... stars, which do not fill their inner Roche lobes SD -- semi-detached systems, where ... Stars from the following catalogues will be included in the first version of ISBS ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P2-36.pdf -- 96.0 Кб -- 27.08.2004
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    45. http://www.adass.org/adass/proceedings/adass00/reprints/P1-22.pdf
    ... The plots show the difference between the star centroid and that star's `expected' location. ... star's actual position is well known, one can use the spacecraft motion described by the aspect solution to predict where that ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass00/reprints/P1-22.pdf -- 540.4 Кб -- 29.05.2001
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    46. Correction of Systematic Errors in Differential Photometry
    ... consequence, some stars exhibit large time variations (see the light curve of star b ... These variations are quite different from star to star. ... stars at the edge of the CCD are too bright by about 0.05mag relative to the stars ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass00/P1-03/ -- 16.3 Кб -- 29.05.2001
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    47. ADASS 2003 Conference Proceedings
    ... stars remains hampered by the lack of statistics and only a few hundred stars with M ... stars a relatively easy job: therefore, we can hope to increase our knowledge of ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass03/P10-2/ -- 13.2 Кб -- 13.08.2004
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    48. Deconvolution as a Tool for Improved Crowded-Field Photometry with HST
    ... stars which are ``neighbors" to the PSF stars; while around bright stars, both these ... star detection on sub-sampled MEM - deconvolved images, because the actual complex ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass99/P2-49/ -- 16.1 Кб -- 05.10.2000
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    49. ADASS 2003 Conference Proceedings
    ... Stars from the following catalogues will be included in the first version of ISBS: Catalog of orbital elements, masses and luminosities of close double stars (Svechnikov & Bessonova 1984); The catalogue of approximate photometric and absolute elements of ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass03/P2-36/ -- 15.0 Кб -- 13.08.2004
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    50. http://www.adass.org/adass/proceedings/adass94/smirnovo1.ps
    ... Each star list is an ASCII table with one line per star. ... Calibrate produces a simulated star field by plotting the stars of a list on an ... 3 only faint stars are measured by DAOPHOT II, the brighter stars be­ ing saturated ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass94/smirnovo1.ps -- 116.8 Кб -- 13.06.1995
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