The data reduction technique is based on Rufener's method of variable principal extinction coefficients, which is applied to the photoelectric RGU-system to determine accurate extraterrestrial G-magnitudes and (G-R) and (U-G)-colors of a first set of standard stars.
Peak
Filter Name wavelength Width
[Å] [Å]
R : Balzer K-65 filtraflex 6550 490
G : special + 2 mm Schott BG13 4650 500
U : Balzer K-36 filtraflex 3650 440