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Match Criteria for Automatic Alignment of Normal Astrograph and Schmidt Plate

Published online by Cambridge University Press:  03 August 2017

A. Fresneau
A. Fresneau*
Affiliation:
Observatoire astronomique, 11, Rue de l'Université, 67000 Strasbourg, France

Abstract

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The objective of the present study is to clarify the tests, checks and clues one may employ to determine whether a feature on a one century old plate is probably identical to a feature on a recent Schmidt plate. A test region of 40′ × 40′ around star HD 42088 was selected in order to detect a variability in nebulosities around Gem OB 1 stars.

Type
Part II: Current Research
Information
Symposium - International Astronomical Union , Volume 133: Mapping the Sky: Past Heritage and Future Directions , 1988 , pp. 207 - 210
Copyright
Copyright © Kluwer 1988 

References

– Fresneau, A. 1987, Bull. Inform. CDS 32, p. 21 Google Scholar
– Groth, E. 1986, Astron. J. 91(5), 1244 Google Scholar
– Humphreys, R.M., 1987, Visitor Use of the APS at the University of Minnesota (Department of Astronomy, Minneapolis)Google Scholar
– Papadimitriou, C.H., Steiglitz, K., 1982, Combinatorial optimization, Prentice Hall Google Scholar