5 Summary

For evolved G and K stars, metallicity calibrations have been derived for $\delta$CN and three other L-R parameters. For G and K dwarfs, two calibrations have been obtained. For metallicities obtained from the calibrations, rms errors turn out to be comparable to those for averaged H-D results. No pair of calibrations is found for which averaging of results definitely yields improved rms errors.

Acknowledgements

I thank Mike and Lisa Joner for carefully proofreading this paper. Page charges for this and the other papers in this series have been generously underwritten by the College of Physical and Mathematical Sciences and the Physics and Astronomy Department of Brigham Young University.