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Progress Report on the Southern Proper Motion Program

Published online by Cambridge University Press:  07 August 2017

I. Platais
Affiliation:
Yale University Observatory P.O. Box 208101, New Haven, CT 06520, U.S.A.
T. M. Girard
Affiliation:
Yale University Observatory P.O. Box 208101, New Haven, CT 06520, U.S.A.
V. Kozhurina-Platais
Affiliation:
Yale University Observatory P.O. Box 208101, New Haven, CT 06520, U.S.A.
R. A. Mendez
Affiliation:
Yale University Observatory P.O. Box 208101, New Haven, CT 06520, U.S.A.
W. F. Van Altena
Affiliation:
Yale University Observatory P.O. Box 208101, New Haven, CT 06520, U.S.A.
C. E. Lopez
Affiliation:
Felix Aguilar Observatory 5413 Chimbas, San Juan, Argentina
W. Z. Ma
Affiliation:
Beijing Normal University Observatory Beijing 100875, China

Extract

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We present the status of the Yale/San Juan Southern Proper Motion program (SPM) which is the southern hemisphere extension of the Lick Observatory Northern Proper Motion program with respect to faint galaxies (Platais et al., 1993). To date, measurements and reductions in the South Galactic Pole region comprising ≈ 1000 square-degrees on the sky have been finished. At this stage of the SPM program particular attention has been paid to the plate model choice along with an assessment of and accounting for systematic errors. For our establishing of a secondary reference frame we have noticed the presence of a potentially dangerous effect, so–called field–independent coma which is caused by lens decentering. We acknowledge the superb Hipparcos preliminary positions without which such analysis would be virtually impossible. The SPM data at the SGP region have also been used to constrain a multi–component Galaxy model. First results of this analysis are presented.

Type
Posters
Copyright
Copyright © Kluwer 1995 

References

Platais, I., Girard, T.M., van Altena, W.F., López, C.E. (1993) in Workshop on Databases for Galactic Structure, eds. Davis Philip, A.G., Hauck, B. and Upgren, A.R., p. 153.Google Scholar