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2015
DOI: 10.1016/j.solmat.2015.03.008
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Impact of Cu–Au type domains in high current density CuInS 2 solar cells

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Cited by 15 publications
(19 citation statements)
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“…The dominant peak at 294.4 cm −1 in the spectrum of x = 1.00 can be assigned to A 1 (Itrue4¯2d) mode of CuInS 2 phase . Peaks at 243.5 and 339.8 cm −1 are almost consistent with the reported values of CuInS 2 .…”
Section: Resultssupporting
confidence: 80%
“…The dominant peak at 294.4 cm −1 in the spectrum of x = 1.00 can be assigned to A 1 (Itrue4¯2d) mode of CuInS 2 phase . Peaks at 243.5 and 339.8 cm −1 are almost consistent with the reported values of CuInS 2 .…”
Section: Resultssupporting
confidence: 80%
“…The 195 cm −1 contribution can possibly be attributed to the Cu–Au Cu(In,Ga)Se 2 structure (space group P4Mtrue¯2), showing similitudes with the very copper‐poor CuInS 2 case. [ 21 ] This would however be, to our knowledge, the first time that such phase is reported in Ga‐rich CIGSe samples, and caution should thus be exercised.…”
Section: Resultsmentioning
confidence: 83%
“…In thin film photovoltaics, a rigorous control of the optoelectronic properties of the growing layers is of major importance in terms for good reproducibility and homogeneity. We have shown in previous works that advanced Raman spectroscopy can assess relevant properties in photovoltaic materials such as film thickness24, crystal structure25, defect densities26, composition272829 and how it can be used as a versatile and fast tool for quality control and process monitoring24.…”
mentioning
confidence: 99%