I. Introduction
Initially presented as memory solutions [1] , [2] , Charge Coupled Devices (CCDs) have found a niche as imaging detectors due to their ability to obtain high resolution digital images. In particular, scientific CCDs have been extensively used in ground and space-based astronomy and X-ray imaging [3] . CCDs have low read-out noise, good spatial resolution, and low dark current. Furthermore, CCDs can be made thick and fully-depleted to increase its detection mass, enabling their use as particle detectors [4] . The low read-out noise can be as low as 2 e − , which enables obtaining a low energy threshold of 5.5 eV. Recently, with the development of fully-depleted Skipper-CCD, it has been possible to achieve a extremely low readout noise of 0.068e − [5] , [6] . Currently, the Sub-Electron-Noise Skipper-CCD Experimental Instrument (SENSEI) will use ~50 skipper-CCD to achieve a 100 gram mass for dark matter searches [7] . Other experiments like CONNIE (Coherent Neutrino-Nucleous Interaction Experiment) [8] and DAMIC (Dark Matter in CCDs) [9] are planning to migrate to this new skipper-CCD technology. This context has motivated the development of a low-noise electronic controller for Skipper-CCD, which will ease the migration for the mentioned experiments. The design of the so called Low-Threshold Acquisition (LTA) system is presented in Section II . Experimental results obtained with Skipper-CCD are shown in Section III , and Section IV summarizes and concludes the work.