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The nomenclature of a recent paper by C. Candler on this subject differs from that of the revised C. E. K. Mees’s “Theory of the Photographic Process” and neither adopts a long-established usage in stellar spectrophotometry. The best-known formulae are here shown to be special cases of a more generally applicable formula deduced from plausible assumptions, and a compromise notation is suggested.
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Ellen Baker (1957) studied this question.
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