Abstract
AbstractObserved 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.
Publisher
Cambridge University Press (CUP)
Reference36 articles.
1. Taylor B. T. , 1984, Astrophys. J. Suppl., 54, 167.
2. Straizys V. and Sviderskiene Z. , 1972, Bull. Vilniuis Obs., No. 35, 3.
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