RGB (Indonesian Wikipedia)

Analysis of information sources in references of the Wikipedia article "RGB" in Indonesian language version.

Last modified:

Ref.Un. Ref.Website
Global rank Indonesian rank
6th place
3rd place
3rd place
4th place
2nd place
2nd place
263rd place
373rd place
1st place
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low place
low place

archive.org (Global: 6th place; Indonesian: 3rd place)

  • Fairman, Hugh S.; Brill, Michael H.; Hemmendinger, Henry (Februari 1997). "How the CIE 1931 color-matching functions were derived from Wright-Guild data". Color Research & Application. 22 (1): 11–23. doi:10.1002/(SICI)1520-6378(199702)22:1<11::AID-COL4>3.0.CO;2-7. The first of the resolutions offered to the 1931 meeting defined the color-matching functions of the soon-to-be-adopted standard observer in terms of Guild's spectral primaries centered on wavelengths 435.8, 546.1, and 700nm. Guild approached the problem from the viewpoint of a standardization engineer. In his mind, the adopted primaries had to be producible with national-standardizing-laboratory accuracy. The first two wavelengths were mercury excitation lines, and the last named wavelength occurred at a location in the human vision system where the hue of spectral lights was unchanging with wavelength. Slight inaccuracy in production of the wavelength of this spectral primary in a visual colorimeter, it was reasoned, would introduce no error at all.{{cite journal}}: Pemeliharaan CS1: Tanggal diterjemahkan otomatis (link)
  • R. W. G. Hunt (2004). The Reproduction of Colour (Edisi 6th). Chichester UK: Wiley–IS&T Series in Imaging Science and Technology. ISBN 0-470-02425-9.

books.google.com (Global: 3rd place; Indonesian: 4th place)

doi.org (Global: 2nd place; Indonesian: 2nd place)

  • Fairman, Hugh S.; Brill, Michael H.; Hemmendinger, Henry (Februari 1997). "How the CIE 1931 color-matching functions were derived from Wright-Guild data". Color Research & Application. 22 (1): 11–23. doi:10.1002/(SICI)1520-6378(199702)22:1<11::AID-COL4>3.0.CO;2-7. The first of the resolutions offered to the 1931 meeting defined the color-matching functions of the soon-to-be-adopted standard observer in terms of Guild's spectral primaries centered on wavelengths 435.8, 546.1, and 700nm. Guild approached the problem from the viewpoint of a standardization engineer. In his mind, the adopted primaries had to be producible with national-standardizing-laboratory accuracy. The first two wavelengths were mercury excitation lines, and the last named wavelength occurred at a location in the human vision system where the hue of spectral lights was unchanging with wavelength. Slight inaccuracy in production of the wavelength of this spectral primary in a visual colorimeter, it was reasoned, would introduce no error at all.{{cite journal}}: Pemeliharaan CS1: Tanggal diterjemahkan otomatis (link)

imaging.org (Global: low place; Indonesian: low place)

microsoft.com (Global: 263rd place; Indonesian: 373rd place)

learn.microsoft.com

web.archive.org (Global: 1st place; Indonesian: 1st place)