Optical parameters of Cu(In,Ga)Se 2 (CIGS) thin fi lms were determined by measuring optical transmission and refl ectance spectra at room temperature. CIGS thin fi lms with average Ga/(Ga + In) ratio ~0.45 were deposited on glass substrates using a three-stage process. The fi lms had thickness d ~ 1.6 μm and refractive index n ~ 2. 38-2.53 in the transparency range. The band-gap energy E g of the CIGS thin fi lms was ~1.36 eV at 293 K. The infl uence of chemical composition heterogeneity along the depth of the absorbing layers on the spectral position of the fundamental absorption edge of the CIGS solid solutions was discussed.Introduction. Optical properties of group I-III-VI 2 semiconductors with the chalcopyrite structure have recently been actively investigated because of their potential use to fabricate highly effi cient solar-energy collectors [1][2][3]. The most signifi cant practical result was the fabrication of solar cells of CuIn 1-x Ga x Se 2 (CIGS) solid solutions with effi ciencies η ~ 19.0-20.3% [1-6]. These effi ciencies are some of the highest for known thin-fi lm semiconductor solar-energy collectors [1,3,4]. In particular, the most similar competitive solar cells that represent an alternative to those based on CIGS solid solutions are based on simpler semiconductors and have lower effi ciencies, e.g., CdTe, η ~ 18.3%; amorphous α-Si:H, η ~ 16.1%; and nanocrystalline Si (nc-Si), η ~ 10.1% [6]. It was shown [5] that η ~ 19.0-19.5% can be achieved in solar cells for defi nite ratios of In and Ga substituents in CIGS solid solutions that vary in the ranges 0.21 < Ga/(Ga + In) < 0.38 and for metal ratios 0.69 < Cu/(Ga + In) < 0.98. Furthermore, improved effi ciency for CIGS solar cells as fi lms with a wide bandgap (E g ~ 1.20-1.45 eV) was recently demonstrated and was characteristic for the composition x = Ga/(Ga + In) > 0.3 [1]. This signifi cantly expanded the technical potential of highly effi cient solar cells compared with the previously achieved η ~ 19.9% for x = 0.3 and E g ~ 1.1-1.2 eV [4]. In particular, η ~ 16 and >18% for E g ~ 1.45 and 1.30 eV for thin-fi lm CIGS solar cells [1]. Therefore, further progress in fabricating CIGS solar cells may be related to obtaining more detailed information on their optical properties (absorption, refl ectance, luminescence, etc.) near the fundamental absorption edge of solid solutions with x > 0.3. New data on important characteristics such as the refractive index and absorption and refl ection coeffi cients near the fundamental absorption edge of CIGS solid solutions with a high Ga concentration (x ~ 0.45) are reported in the present work.Experimental. Thin fi lms of CIGS solid solutions were deposited on Na-glass substrates using a three-stage process with high-vacuum thermal vaporization of Cu, In, Ga, and Se from various sources according to the literature method [7]. The fi lm chemical composition was determined by energy-dispersive x-ray microanalysis (EDX), averaging fi ve measurements at various points on the surface, and by scanning Auger m...