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Determination of Absolute Proper Motions by Use of Automated Measurements of Tautenburg Plates

Published online by Cambridge University Press:  19 July 2016

R.-D. Scholz
R.-D. Scholz*
Affiliation:
Central Institute of Astrophysics DDR - 1561 Potsdam Germany, Dem. Rep.

Abstract

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From measurements of Tautenburg Schmidt plates with the APM in Cambridge positional accuracies per plate of 0.″05 for stars and of 0.″10 for galaxies were achieved. With 0.″3/100a accuracy in a single stellar proper motion we obtained the absolute proper motion of the M3 globular cluster in good agreement between the two pairs of plates used.

Type
Part 4: Realization and comparison of reference frames
Information
Symposium - International Astronomical Union , Volume 141: Inertial Coordinate System on the Sky , 1990 , pp. 451 - 452
Copyright
Copyright © Kluwer 1990 

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