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An in situ sulfur four-isotope analysis technique with multiple Faraday cup detectors by ion microprobe was developed and applied to detrital pyrite grains in ~2.4 Ga glaciogenic sandstone from the Meteorite Bore Member of the Turee Creek Group, Western Australia. Data are standardized with the UWPy-1 pyrite standard (δ³⁴S =16.04 ± 0.18‰, Δ³³S = −0.003 ± 0.009‰, and Δ³⁶S = −0.21 ± 0.24‰, 2 SD) whose sulfur four isotopes were newly determined by gas-source mass spectrometry. Typical reproducibility at two standard deviations (2 SD) of spot-to-spot analyses of standard UWPy-1 pyrite with a primary beam size of ~20 μm were ±0.23, ±0.05, and ±0.86‰ for δ³⁴S, Δ³³S, and Δ³⁶S, respectively. The measured ³⁶S/³²S ratio [1 / (6641 ± 27)] is approximately 19‰ lower than the published ratio for VCDT, and we propose a revision of the ³⁶S abundance in VCDT. Pyrite grains in ~2.4 Ga glaciogenic sandstone have wide ranging sulfur isotope ratios (−32.7 to 13.5 for δ³⁴S, −3.03 to 11.66 for Δ³³S, and−9.7 to 4.6 for Δ³⁶S, respectively). Some pyrite grains are zoned in δ³⁴S values within a grain. Sulfur isotope ratios of most pyrite grains are distributed along a line with slope = −0.9 for Δ³³S vs. Δ³⁶S, suggesting that pyrite grains mostly derived from a limited range of source rocks and near-surface sulfur reservoirs. One pyrite aggregate has a distinct texture from other pyrite grains in the same sandstone, and yields a significant mass-independent deficit in ³⁶S with a small excess in ³³S (Δ³⁶S/Δ³³S ~−4‰). This is used to suggest that this grain authigenically formed by biological activity during or after sedimentation. This work demonstrates that the use of multiple Faraday cup detectors provides improved accuracy and precision for in situ sulfur four isotope analysis with secondary ion mass spectrometry.