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    1. ADASS 2003 Conference Proceedings
    ... 1 . Introduction . 2 . Observation of asteroids and satellites . 3 . ... 3 . Algorithm for asteroids and satellites astrometry . 4 . Fields comparison . 5 . ... University (OAUV), CCD observations of asteroids and big planets satellites are ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass03/P6-2/ -- 12.7 Кб -- 27.08.2004
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    2. http://www.adass.org/adass/proceedings/adass03/reprints/P6-2.pdf
    ... step of the asteroid identification We have developed algorithms for several kinds of observations, including ephemerids calculation, stellar maps presentation, measuring and reduction of CCD fields and residuals calculation for asteroids observations ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/P6-2.pdf -- 705.5 Кб -- 27.08.2004
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    3. ADASS 2003 Conference Proceedings
    ... Next: Images analysis in Asteroid and Satellites Astrometry . Up: Surveys, Archives & VO . ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass03/P6-1/ -- 23.8 Кб -- 14.08.2004
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    4. ADASS 2003 Conference Proceedings
    ... Up: Surveys, Archives & VO . Previous: Images analysis in Asteroid and Satellites Astrometry . ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass03/P6-3/ -- 10.2 Кб -- 27.08.2004
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    5. Modern CCD Observations of Moving Celestial Objects: Algorithms and Software
    ... The problems of observing asteroids using CCDs are discussed. ... obtain several hundreds of thousands of asteroid positions and send them to the ... for the MPC to receive observations of asteroids with their identifications ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass98/bykovo/ -- 12.3 Кб -- 16.07.1999
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    6. A New Stable Method for Long-Time Integration in an N-Body Problem
    ... We tested this method for several astronomical systems and for motion of an asteroid in a 1:1 Jupiter resonance during 200 million time steps (about 5 million years or 800 thousand periods of asteroid resonance motion). ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/taidakovat.html -- 9.4 Кб -- 23.06.1998
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    7. A Computer-Based Technique for Automatic Description and Classification of
    ... all of the variety of the asteroid polarization phase dependencies (Vasilyev 1994 ... In the case of asteroids, the method allows the synthesis of the polarization curves ... components of the family of asteroid polarimetric phase curves have physical ...
    [ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/vasilyevs.html -- 11.6 Кб -- 23.06.1998
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    8. http://www.adass.org/adass/proceedings/adass96/reprints/taidakovat.pdf
    ... We tested this method for several astronomical systems and for motion of an asteroid in a 1:1 Jupiter resonance during 200 million time steps (ab out 5 million years or 800 thousand p eriods of asteroid resonance motion). ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass96/reprints/taidakovat.pdf -- 151.3 Кб -- 14.01.1998
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    9. http://www.adass.org/adass/proceedings/adass96/reprints/vasilyevs.pdf
    ... e all of the variety of the asteroid p olarization phase dep endencies (Vasilyev ... In the case of asteroids, the method allows the synthesis of the p olarization ... comp onents of the family of asteroid p olarimetric phase curves have physical ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass96/reprints/vasilyevs.pdf -- 108.5 Кб -- 14.01.1998
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    10. http://www.adass.org/adass/proceedings/adass03/reprints/O1-3.pdf
    ... lensing, supernovae and GRBs, and near-Earth asteroids and trans-Neptunian ob jects ... moving ob jects (e.g. asteroids) · optimally characterizing the variability of an ob ...
    [ Текст ]  Ссылки http://www.adass.org/adass/proceedings/adass03/reprints/O1-3.pdf -- 156.0 Кб -- 27.08.2004
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