2015
DOI: 10.1002/col.21951
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Testing the accuracy of methods for the computation of CIE tristimulus values using weighting tables

Abstract: The least squares method for computing colorimetric weighting tables is presented and its connection with the optimum weights method is investigated. Each requires solving three linear systems of equations with the same coefficient matrix but three different right hand side vectors. It is shown that the two methods have nearly the same performance when the wavelength interval of the data is large. The two methods however, will perform differently when Δλ is small. Comparisons are also made between the least sq… Show more

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Cited by 9 publications
(18 citation statements)
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“…The spectral bandpass function. 10 the deficiencies of the instruments through mathematical methods so as to improve the accuracy of the TSVs.…”
Section: Methods For Higher Accuracy Of Tsvsmentioning
confidence: 99%
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“…The spectral bandpass function. 10 the deficiencies of the instruments through mathematical methods so as to improve the accuracy of the TSVs.…”
Section: Methods For Higher Accuracy Of Tsvsmentioning
confidence: 99%
“…At present, ASTM provides 36 weighting tables in 360-780 nm range at 10and 20-nm intervals under illuminates of A, C, D, and F. Since there is no relative paper publish the detail of its algorithm, the specific processing method has been lost. 10 Therefore, this method can only be used for the given illuminates and observers. Table LLR and Table LWL provide simple ways to generate weighing tables according to equation (15); hence, it is easy to derive other tables for any intervals, any ranges, any illuminants, and any observers.…”
Section: Reduce Bandpass Error By Bandpass Correctionsmentioning
confidence: 99%
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“…Coordinates u, v of the test light source (or illuminant) must also be computed from accurate TSVs using CIE recommendation (summations from 360 nm to 830 nm at 1 nm steps). Some methods have been recently proposed [24,25] for accurate TSVs computations in the case available spectral data are not as required by CIE. For the function f(T), the exact u(T) and v(T) are needed, which depend on the TSVs X(T), Y(T) and Z(T) (see Eqs. (5), (3), and (2)).…”
Section: The Proposed Methodsmentioning
confidence: 99%
“…Then, this set of reflectance functions was also extrapolated to cover the range from 360 to 830 nm. Thus, altogether, we constituted a dataset with 2365 SRFs at 1‐nm intervals from 360 to 830 nm, which provides a reasonable good coverage of the color gamut of real object colors and is referred to in this article as the standard dataset. For the purposes of the calculations to be described in this article, the accuracy of the measurements in our standard dataset is not of importance; it is enough that a set of realistic spectral data are available.…”
Section: Datasetmentioning
confidence: 99%