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Statistical Problems Encountered in Using Trigonometric Parallaxes

Published online by Cambridge University Press:  04 August 2017

Thomas E. Lutz
Thomas E. Lutz*
Affiliation:
Program in Astronomy, Washington State University

Extract

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The importance of understanding the properties of a data sample which is to be used for calibrating luminosities can hardly be overemphasized. In an earlier paper (Lutz 1983) I pointed out the methods for dealing with two well-defined cases. In this paper I will elaborate further on the same topic.

Type
I. Reduction Technique
Information
Symposium - International Astronomical Union , Volume 109: Astrometric Techniques , 1986 , pp. 47 - 52
Copyright
Copyright © Reidel 1986 

References

Lutz, T. E.: 1979, Monthly Notices Roy. Astron. Soc. 189, pp. 273–278.CrossRefGoogle Scholar
Lutz, T. E.: 1983, In “Nearby stars and the Stellar Luminosity Function”, IAU Coll. No. 76, eds. Phillip, A. G. D. and Upgren, A. R., Van Vleck Observatory, Middletown, pp. 41–49.Google Scholar
Lutz, T. E. and Kelker, D. H.: 1973, Pub. Astron. Soc. Pacific 85, pp. 573–578.Google Scholar
Malmquist, K. G.: 1920, Lund Astron. Obs. Medd., Ser. II, No. 22.Google Scholar
Malmquist, K. G.: 1936, Stockholm Obs. Medd., No. 26.Google Scholar