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Observed Stellar Energy Distributions for Synthetic Photometry
Published online by Cambridge University Press: 30 March 2016
Abstract
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
- Information
- Copyright
- Copyright © Reidel 1986
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