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

Published online by Cambridge University Press:  25 May 2016

George A. Goncharov
George A. Goncharov*
Affiliation:
Pulkovo observatory 196140, Saint-Petersburg, Russia

Extract

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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).

Type
Part X - Solar System Astrometry
Information
Symposium - International Astronomical Union , Volume 172: Dynamics, Ephemerides and Astrometry of the Solar System , 1996 , pp. 435 - 436
Copyright
Copyright © Kluwer 1996 

References

Høg, E. (1968) Refraction anomalies: the mean power spectrum of star image motion, Zeitschrift für Astrophisik, Vol. 69, pp. 313–325 Google Scholar
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. 103–108 Google Scholar
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. 3–8 CrossRefGoogle Scholar