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Observed Stellar Energy Distributions for Synthetic Photometry

Published online by Cambridge University Press:  30 March 2016

D. S. Hayes*
Affiliation:
Kitt Peak National Observatory, National Optical Astronomy Observatories, P. O. Box 26732, Tucson, Arizona, U.S.A. 85726

Abstract

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Observed stellar energy distributions are used in synthetic photometry to evaluate the accuracy of the response functions and to determine the transformation coefficients. The characteristics required of a catalog of energy distributions to be used for synthetic photometry are discussed, and the catalogs found in the literature are reviewed.

Type
Synthetic Photometry
Copyright
Copyright © Reidel 1986

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