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The Buying Power of High Signal-to-Noise Ratios in Spectroscopy

Published online by Cambridge University Press:  19 July 2016

David F. Gray
David F. Gray*
Affiliation:
Department of Astronomy, University of Western Ontario, London, Ontario, Canada N6A 3K7

Abstract

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High S/N is a good first step toward accurate profiles.

Type
IV. Spectroscopic Patterns of Stellar Atmospheres
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 185 - 191
Copyright
Copyright © Kluwer 1988 

References

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