To fully exploit the potential of a 2-junction photovoltaic (PV) tandem device, the top cell should exhibit an absorber bandgap energy (E g ) above 1.4 eV in a 4-terminal and E g % 1.6 eV in a 2terminal configuration. [1,2] Such high bandgaps can be reached for Cu(In,Ga)Se 2 (CIGS) films with [Ga]/([Ga]þ[In]) (GGI) values > 0.6. However, while efficiencies (η) of CIGS-based solar cells exceed 22% for GGI values ≤ 0.3, [3,4] a distinctly inferior performance is observed for wide-gap chalcopyrite solar cells with higher Ga contents (i.e., E g > 1.2 eV). [5] The most prominent bottleneck is the increasing open-circuit voltage (V OC ) deficit with respect to the bandgap energy. While some of the large V OC loss of wide-gap chalcopyrite solar cells can be mitigated by using alternative (i.e., not CdS) buffer layers with tunable electron affinity (χ), [6][7][8][9][10] a major part of the deficit seems to arise from a poorer bulk quality. [11,12] The lifetime deterioration with increasing GGI was suggested to originate from higher Shockley-Read-Hall (SRH) recombination via 1) energetically deeper Ga Cu antisite donor defects [13][14][15][16] or (V Se -V Cu ) complexes in acceptor state [17] ; 2) an increasing density of deep acceptors [18,19] ; 3) an increasing tetragonal lattice distortion [20] ; and/or 4) an increased fraction of Cu-enriched (supposedly detrimental [21] ) grain boundaries (GBs). [22] Instead of utilizing low-χ alternative buffers, interface recombination can also be reduced (or canceled out) for CdS-buffered wide-gap CIGS solar cells when the absorber is alloyed with silver, i.e., forming (Ag,Cu)(In,Ga)Se 2 (ACIGS). While a detrimental negative conduction band offset (CBO) at the CdS/CIGS interface is predicted for GGI > 0.5, [23][24][25] sufficient Ag-alloying allows to avoid a negative CBO in the entire compositional range of ACIGS (i.e., even for GGI ¼ 1). [7,26,27] Consequently, high V OC values close to 900 mV and beyond were achieved for wide-gap ACIGS solar cells with CdS buffer layers by several groups. [7,11,[28][29][30][31][32] However, it was reported that the chalcopyrite single-phase region of the ACIGS system is narrowing toward GGI and AAC ¼ 1 (i.e., AgGaSe 2 ). [33] As a result, a high volume share of ordered vacancy compound (OVC) patches is observed, which significantly increases for AAC and GGI > 0.5. [7,31,34,35] While OVCs at the back contact very likely cause a kink in current-voltage (I-V ) characteristics and thus a low fill factor (FF), it is currently not clear whether their occurrence at the heterojunction is beneficial, detrimental, or benign. [11,31] Further studies are ongoing to investigate the effect of the OVC patches on the electrical and optical properties of the ACIGS devices.Recently, we revealed a clear anticorrelation between V OC and the short-circuit current density ( J SC ) with varying group-I stoichiometry for wide-gap ACIGS solar cells. [11] Perfect carrier collection (high J SC ) is only achieved for very close-stoichiometric compositions, due to a complet...