Skipper-CCDs, with their electron-counting capability and low instrumental background, are highly sensitive to faint signals, which is of great interest for certain astronomical applications. Characterizing the instrumental sources of few-e- events in skipper-CCDs is crucial for estimating their scientific reach. In this work I will report on the performance of fully-depleted, p-channel skipper-CCDs, that were fabricated on 8-inch wafers in two new foundries during the R&D of Oscura, a 26 GPix skipper-CCD array designed to search for light dark matter-electron interactions. Results, performed at FNAL, demonstrate a high yield of sensors achieving sub-electron readout noise. Main instrumental sources of few-e- events were identified and characterized, including thermal dark current, spurious charge and charge traps.
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