Cu(In,Ga)Se 2 (CIGS)-based thin film solar cells hold significant promise due to the tunable, direct bandgap, high absorption coefficient, thin layers, flexible and rigid substrate applications, processing options, and consistent efficiency increases. [1][2][3] Photovoltaic conversion efficiencies have reached 23.4% in small-area CIGS solar cells, [4] and significant improvements have originated from absorber composition changes and heavy alkali postdeposition treatments (PDTs). [5][6][7][8][9][10][11][12][13] The absorber energy gap and electron affinity can be controlled by the Ga/(GaþIn) (GGI) ratio, which offers two benefits. First, increases in GGI widen the absorber bandgap which raises the maximum achievable open circuit voltage (V OC ) and efficiency of the device. [14] Second, GGI grading is used to create a "notched" graded bandgap in which the bandgap is increased at both the front and rear portions of the absorber, and a bandgap minimum is maintained in the front half of the absorber. [6] The front-side bandgap increase reduces front interface hole recombination and back-side grading reduces back interface electron recombination such that V OC improvements up to 100 mV are achievable with a change in GGI %0.5. [15,16] However, voltage losses increase for GGI > 0.4 in the minimum bandgap region such that efficiency improvements are limited. [17][18][19] This can be mitigated in part through silver-alloyed ACIGS devices ((Ag,Cu)(In,Ga)Se 2 ), which