IMPORTANT INFORMATION:
Please, register as soon as possible through the registration form. The CYGNO Collaboration Meeting 2026 participation is completely free of charge, but we need to know how many people will come in person and visit Laboratori Nazionali del Gran Sasso as soon as possible for organisational reasons.
SITE UNDER CONSTRUCTION, STAY TUNED!
CYGNO COLLABORATION MEETING 2026
The CYGNO experiment (a CYGNus module with Optical readout) aims at exploiting the optical readout approach of multiple-GEM structures in large volume TPC for the study of rare events as interactions of low mass Dark Matter or Solar Neutrinos. The combined use of high-granularity sCMOS camera and fast light sensors allows the reconstruction of the 3D direction of the tracks, offering good energy resolution and very high sensitivity in the few keV energy range, together with a very good particle identification useful to distinguish nuclear recoils from electronic recoils. This experiment is part of the CYGNUS proto-collaboration which aims at establishing a multi-site multi-target Galactic Directional Recoil Observatory to probe the Dark Matter hypothesis below the Neutrino Floor and measure Solar Neutrinos with directionality.
Local Organising Committee
Elisabetta Baracchini
Davide Fiorina
Stefano Piacentini
Davide Pinci
Giuseppe Oppedisano
