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CCD astrometry oriented analysis of digitized multiple images (planets, satellites, etc.) obtained with the Pulkovo PVC

  • George A. Goncharov (a1)
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The Charge Coupled Device (CCD) has become the detector of choice in astrometry. The mechanical or electronic (drift scanning) tracking of objects by the telescope leads among observing strategies developed for CCD observations (Stone and Dahn, 1995).

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      CCD astrometry oriented analysis of digitized multiple images (planets, satellites, etc.) obtained with the Pulkovo PVC
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      CCD astrometry oriented analysis of digitized multiple images (planets, satellites, etc.) obtained with the Pulkovo PVC
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References
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Høg, E. (1968) Refraction anomalies: the mean power spectrum of star image motion, Zeitschrift für Astrophisik, Vol. 69, pp. 313325
Schildknecht, T., Hugentobler, U., Verdun, A. (1994) CCD astrometry of artificial satellites, In Dynamics and Astrometry of Natural and Artificial Celestial Bodies, (Kurzyńska, K. et al., Eds), Poznań, pp. 103108
Stone, R.C., and Dahn, C.C. (1995) CCD astrometry, In Proc. of the IAU Symp. No. 166, Astronomical and Astrophysical Objectives of Sub-Milliarcsecond Optical Astrometry (Høg, E. and Seidelmann, P. K., Eds), Kluwer Acad. Publ., pp. 38
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Proceedings of the International Astronomical Union
  • ISSN: -
  • EISSN: 0074-1809
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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