Concept

The Judd–Vos correction — where it appears

A correction to the 1931 observer's short-wave end, which is known to be too low. It gives better agreement with matching data below about 460 nanometres and is not what any colour specification is written in, so it exists as a known repair nobody applies.

Named by 2 essays across one field — each of them below, with the objects they name alongside it.

Named alongside it

The objects these essays reach for when they reach for this one.

Colour-matching functionsMacular pigmentObserver metamerismStandard observerXYZChromaticityThe CIE 1931 2° observerThe CIE 1964 10° observerCone fundamentalsIndividual variationPrimariesWhite point

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