Astrometric investigation with the Tautenburg Schmidt Telescope

Details Astrometric investigation with the Tautenburg Schmidt Telescope Astrometric investigation with the Tautenburg Schmidt Telescope

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.177..229d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 177, no. 1-2, March 1991, p. 229-234.

Astronomy and Astrophysics

Astrophysics

1

Astrometry, Schmidt Telescopes, Stellar Motions, Accuracy, Astronomical Photography, Error Analysis, Faint Objects, Reference Stars, Transits

Scientific paper

The observations and the plate reduction technique for the determination of positions and absolute proper motions which is used in Potsdam are described. Recent results have shown that an accuracy of about 0.1 arcsec for positions and 0.7 arcsec/cent for proper motions can be achieved both for bright (8-12 mag) and faint (16-18 mag) stars. Three astrometric programs using the Tautenburg plates are presented.

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