“…The chemical composition and bonding states of the IGZO:O I , IGZO:O II , and IGZO:N were accurately characterized by X‐ray photoelectron spectroscopy (XPS) using monochromatic Ag L α (2984.2 eV) X‐ray source, where the commonly detected Ga LMM Auger peaks by conventional Al K α and Mg K α X‐ray sources that overlapped with N 1s peak are completely removed (Figure 1b,c and Figure S1, Supporting Information). [
26,27 ] Experimentally, the front‐channel IGZO:O I was sputtering grown by pure argon with an optimized flow rate ≈10.00 sccm, which produced heavy O‐deficient IGZO with both high content of V O (
≈26.7%, Figure 1d) and large Hall N e (≈5.2 × 10 19 cm –3 ) and μ (≈93.1 cm 2 V −1 s −1 ). Much higher I on and μ FE would be induced by artificially increasing N e in the space charge region.…”