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Determination of the Apparent V Magnitudes

Published online by Cambridge University Press:  07 February 2017

F. Rufener  and
A. Maeder
F. Rufener
Affiliation:
Geneva Observatory, Switzerland
A. Maeder
Affiliation:
Geneva Observatory, Switzerland

Abstract

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V photoelectric magnitudes are determined on an independent basis. Correlation with V sequence of the UBV system confirms the coincidence of the two definitions. Comparisons with the Catalogue of Bright Stars revealed that more than 40% of BS stars have an apparent V magnitude with a probable error of .

Type
Part VIII: Choice of Standard Stars
Information
Symposium - International Astronomical Union , Volume 54: Problems of Calibration of Absolute Magnitudes and Temperature of Stars , 1973 , pp. 298 - 301
Copyright
Copyright © Reidel 1973 

References

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