{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,12,9]],"date-time":"2025-12-09T15:50:25Z","timestamp":1765295425199,"version":"3.37.3"},"reference-count":5,"publisher":"IOP Publishing","issue":"09","license":[{"start":{"date-parts":[[2023,9,15]],"date-time":"2023-09-15T00:00:00Z","timestamp":1694736000000},"content-version":"vor","delay-in-days":14,"URL":"http:\/\/creativecommons.org\/licenses\/by\/4.0\/"},{"start":{"date-parts":[[2023,9,15]],"date-time":"2023-09-15T00:00:00Z","timestamp":1694736000000},"content-version":"tdm","delay-in-days":14,"URL":"https:\/\/iopscience.iop.org\/info\/page\/text-and-data-mining"}],"content-domain":{"domain":["iopscience.iop.org"],"crossmark-restriction":false},"short-container-title":["J. Inst."],"published-print":{"date-parts":[[2023,9,1]]},"abstract":"Abstract<\/jats:title>\n We are going to discuss the R&D and the prospects for the CYGNO project, towards the\n development of an innovative, high precision 3D tracking Time Projection Chamber with optical\n readout using He:CF4<\/jats:sub> gas at 1 bar. CYGNO uses a stack of triple thin GEMs for charge\n multiplication, this induces scintillation in CF4<\/jats:sub> gas, which is readout by PMTs and sCMOS\n cameras. High granularity and low readout noise of sCMOS along with high sampling of PMT allows\n CYGNO to have 3D tracking with head tail capability and particle identification down to O(keV)\n energy for directional Dark Matter searches and solar neutrino spectroscopy. We will present the\n most recent R&D results from the CYGNO project, and in particular the overground commissioning of\n the largest prototype developed so far, LIME with a 33\u00d733 cm2<\/jats:sup> readout plane and 50 cm of\n drift length, for a total of 50 litres active volume. We will illustrate the LIME response\n characterisation between 3.7 keV and 44 keV by means of multiple X-ray sources, and the data\n Monte-Carlo comparison of simulated sCMOS images in this energy range. Furthermore, we will\n present current LIME installation, operation and data taking at underground Laboratori Nazionali\n del Gran Sasso (LNGS), serving as demonstrator for the development of a 0.4 m3<\/jats:sup> CYGNO\n detector. We will conclude by mentioning the technical choices and the prospects of the\n 0.4 m3<\/jats:sup> detector, as laid out in the Technical Design Report (TDR) recently produced by our\n collaboration.<\/jats:p>","DOI":"10.1088\/1748-0221\/18\/09\/c09010","type":"journal-article","created":{"date-parts":[[2023,9,15]],"date-time":"2023-09-15T14:16:23Z","timestamp":1694787383000},"page":"C09010","update-policy":"https:\/\/doi.org\/10.1088\/crossmark-policy","source":"Crossref","is-referenced-by-count":3,"title":["The CYGNO experiment: a directional Dark Matter detector with optical 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