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  2. Color temperature - Wikipedia

    en.wikipedia.org/wiki/Color_temperature

    Color temperature is a parameter describing the color of a visible light source by comparing it to the color of light emitted by an idealized opaque, non-reflective body. The temperature of the ideal emitter that matches the color most closely is defined as the color temperature of the original visible light source.

  3. Correlated color temperature - Wikipedia

    en.wikipedia.org/wiki/Correlated_color_temperature

    The paper stresses the importance of also returning the Δ uv value for evalulation of light sources. [25] As it does not use one fixed table, it can be applied to any observer color matching function. [26] The inverse calculation, from color temperature to corresponding chromaticity coordinates, is discussed in Planckian locus § Approximation.

  4. G-type main-sequence star - Wikipedia

    en.wikipedia.org/wiki/G-type_main-sequence_star

    The term yellow dwarf is a misnomer, because G-type stars actually range in color from white, for more luminous types like the Sun, to only very slightly yellowish for less massive and luminous G-type main-sequence stars. [7]

  5. Academy Color Encoding System - Wikipedia

    en.wikipedia.org/wiki/Academy_Color_Encoding_System

    Academy Color Encoding Specification (ACES): The specification that defines the ACES color space, allowing half-float high-precision encoding in scene linear light as exposed in a camera, and archival storage in files. Input Device Transform (IDT): This name was deprecated in ACES version 1.0 and replaced by Input Transform.

  6. White - Wikipedia

    en.wikipedia.org/wiki/White

    White light can be generated by the sun, by stars, or by earthbound sources such as fluorescent lamps, white LEDs and incandescent bulbs. On the screen of a color television or computer, white is produced by mixing the primary colors of light: red, green and blue at full intensity, a process called additive mixing (see image above). White light ...

  7. CIE 1931 color space - Wikipedia

    en.wikipedia.org/wiki/CIE_1931_color_space

    A comparison between a typical normalized M cone's spectral sensitivity and the CIE 1931 luminosity function for a standard observer in photopic vision. In the CIE 1931 model, Y is the luminance, Z is quasi-equal to blue (of CIE RGB), and X is a mix of the three CIE RGB curves chosen to be nonnegative (see § Definition of the CIE XYZ color space).

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