Thin films of Cu(In, Ga)Se 2 (CIGS) with a Ga/(Ga + In) ratio of ~0.27 corresponding to the standard elemental composition for solar-energy transducers were grown on Mo-coated glass substrates by the Cu, In, Ga, and Se co-evaporation technique from different sources. Transmission (T), photoluminescence (PL), and photoluminescence excitation (PLE) spectra at 4.2 K were used to analyze electronic properties in the asgrown and electron-irradiated CIGS films. The band-gap energy (E g ) of the CIGS films measured using both transmission and PLE methods was found to be about 1.28 eV at 4.2 K. Two deep bands in the PL spectra of the irradiated CIGS films, P 1 at ~0.91 eV and P 2 at ~0.77 eV, have been detected. These bands are tentatively associated with copper atoms substituting indium (Cu In ) and indium vacancies V In , respectively, as the simplest radiation-induced defects.Introduction. Fabrication of highly efficient solar cells based on Cu(In,Ga)Se 2 (CIGS) semiconducting films is a critical and simultaneously complicated scientific and technical problem of modern semiconducting solar energy [1,2]. The development and improvement of the technology for preparing solar cells using CIGS compounds with the chalcopyrite structure has recently enabled efficiency records (~19.9%) to be set for all known thin-film semiconducting materials [1]. The stable operation of solar cells based on CIGS compounds that are used under ordinary terrestrial conditions and, especially, that are exposed to penetrating radiation (high-energy electrons, protons, etc.) in near-earth space orbits to an even greater extent stimulate further scientific and technological developments of semiconducting solar photovoltaics based on these materials [1][2][3][4][5]. Such promising developments prompt investigations that determine the criteria for radiation resistance of CIGS semiconducting compounds and solar cells based on them to the action of high-energy particles and that establish the nature of the radiation-induced defects at the atomic level [3][4][5][6]. New knowledge about the radiation physics of defects in CIGS material will indubitably assist a deeper understanding of the geometric and electronic structure of not only radiation defects but also growth defects formed during formation of CIGS thin films that determine the perfection of the material crystal structure. Herein we describe experiments that establish the nature of the radiation defects in CdS/Cu(In,Ga)Se 2 /Mo (CdS/CIGS/Mo) heterostructures, on which solar cells with efficiency ~12-14% are based [4,7,8].Experimental. The studied CIGS films were sputtered onto glass substrates coated with a thin film of Mo with simultaneous co-evaporation of Cu, In, Ga,[7][8][9]. Layers of CdS (~50 nm thick) were deposited by the standard chemical method in the corresponding solutions. The studied CdS/CIGS/Mo/glass structures consisted of a CdS buffer layer (~50 nm), CIGS films (~1.5 μm thick), a contact layer of Mo (~0.8 μm thick), and the glass substrate (2 mm thick). The elemental compositio...