Skipper-CCDs: current applications and future
arXiv:2208.05434 · doi:10.1016/j.nima.2022.167681
Abstract
This work briefly discusses the potential applications of the Skipper-CCD technology in astronomy and reviews its current use in dark matter and neutrino experiments. An overview of the ongoing efforts to build multi-kilogram experiments with these sensors is given, in the context of the Oscura experiment. First results from the characterization of Oscura sensors from the first 200 mm wafer-fabrication run with a new vendor are presented. The overall yield of the electron counting capability of these sensors is 71%. A noise of 0.087 e RMS, with 1225 samples/pix, and a dark current of (0.0310.013) e/pix/day at 140 K were measured.
References in corpus (10)
- SENSEI: Direct-Detection Results on sub-GeV Dark Matter from a New Skipper-CCD
- Single-electron and single-photon sensitivity with a silicon Skipper CCD
- Constraints on Light Dark Matter Particles Interacting with Electrons from DAMIC at SNOLAB
- Results on Low-Mass Weakly Interacting Massive Particles from an 11 kg-day Target Exposure of DAMIC at SNOLAB
- Search for light mediators in the low-energy data of the CONNIE reactor neutrino experiment
- DAMIC-M Experiment: Thick, Silicon CCDs to search for Light Dark Matter
- SENSEI: Characterization of Single-Electron Events Using a Skipper-CCD
- The physics potential of a reactor neutrino experiment with Skipper CCDs: Measuring the weak mixing angle
- Search for coherent elastic neutrino-nucleus scattering at a nuclear reactor with CONNIE 2019 data
- The physics potential of a reactor neutrino experiment with Skipper-CCDs: Searching for new physics with light mediators