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Data Analysis

Published online by Cambridge University Press:  19 July 2016

R. Cayrel
R. Cayrel*
Affiliation:
Observatoire de Paris, France

Abstract

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The relationship between the r.m.s. photometric accuracy on the data points of a stellar spectrum and the final accuracy on abundances and physical parameters derived from these data is discussed.

Type
VI. Chemical Composition of Stars
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 345 - 353
Copyright
Copyright © Kluwer 1988 

References

– Kurucz, R.L., Furenlid, I., Brault, J., Testerman, L., 1984, Solar Flux Atlas from 296 to 1300 nm. National Solar Observatory, Sunspot New-Mexico USA Google Scholar
– Landman, D.A., Roussel-Dupre, R., Tanigawa, G., 1982, Astrophys. J. 261, 732.Google Scholar
– Stehle, C., Mazure, A., Nollez, G., Feautrier, N., 1983, Astron. Astrophys. 127, 263.Google Scholar
– Vidal, C.R., Cooper, J., Smith, , 1973, Astrophys. J. Suppl. 25, 37.Google Scholar