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Optical region energy distributions of 13 bright normal B, A, and F stars consistent with the Hayes-Latham calibration of Vega are presented. These scans contain more wavelength values than those given in previous papers in this series. The procedure of synthesizing u-b and b-y values from spectrophotometry is improved. Effective temperatures are found using the empirical calibration of Code and his colleagues and the fully line-blanketed solar composition model atmospheres of Kurucz.
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Adelman et al. (1983) studied this question.
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