Zampieri, LucaLucaZampieri0000-0002-7352-6818Fiori, MicheleMicheleFiori0000-0002-0730-1899Gargano, CarmeloCarmeloGargano0000-0003-3239-6057Lessio, LuigiLuigiLessio0000-0003-4472-4978Rodeghiero, GabrieleGabrieleRodeghiero0000-0002-6311-764XBonanno, GiovanniGiovanniBonanno0000-0002-7752-6268Bruno, PietroPietroBruno0000-0002-3469-9863Naletto, GiampieroGiampieroNaletto0000-0001-6850-2128Paoletti, LorenzoLorenzoPaoletti0000-0001-5570-5081Romeo, GiuseppeGiuseppeRomeoSpolon, AlessiaAlessiaSpolon0000-0002-8637-2109Bulgarelli, AndreaAndreaBulgarelli0000-0003-4666-119XConforti, VitoVitoConfortiGianotti, FulvioFulvioGianotti0000-0002-6336-865XGrillo, AlessandroAlessandroGrillo0000-0001-8770-9503Landoni, MarcoMarcoLandoniLombardi, SaverioSaverioLombardi0000-0002-4792-3983Lucarelli, FabrizioFabrizioLucarelli0000-0002-5284-0656Parmiggiani, NicolòNicolòParmiggiani0000-0001-6347-0649Pernechele, ClaudioClaudioPernechele0000-0002-4535-5329Timpanaro, Maria CristinaMaria CristinaTimpanaro0000-0001-8865-5930Giordano, ValentinaValentinaGiordano0000-0003-3919-9611Pareschi, GiovanniGiovanniPareschi0000-0002-6516-1329Scuderi, SalvatoreSalvatoreScuderi0000-0003-3967-403XTosti, GinoGinoTosti0000-0002-0007-35202024-12-092024-12-092024http://hdl.handle.net/20.500.12386/40703The ASTRI Stellar Intensity Interferometry Instrument (SI3) is a fast single photon counting instrument for performing intensity interferometry observations of bright stars with the ASTRI Mini-Array. SI3 is designed to perform accurate measurements of single photon arrival times (1ns) in a narrow optical bandwidth (1-8nm) centered at a wavelength in the range 420-500nm. The instrument will exploit the 36 simultaneous baselines over distances between 100m and 700m of the ASTRI Mini-Array to achieve angular resolutions below 100 microarcsec. At this level of resolution it turns out to be possible to reveal details on the surface and of the environment surrounding bright stars on the sky. During 2023 SI3 underwent a significant redesign, with an optical fiber positioned on the focal plane to feed the detectors and electronics. Here we present this new baseline design of SI3, and the motivations behind this choice, including the possibility of future upgrades of the instrument with dedicated front-end electronics and channel multiplexing. We will also show the first results of the target selection procedure based on simulations. Stars with angular diameters of less than 500- 600 microarcseconds up to about magnitude 4.5 will be observable. Thanks to the 36 simultaneous baselines, accurate (up to ∼1%) angular measurements can be obtained with 10-30 hours of observations. This accuracy can rival with that obtained with other arrays of Cherenkov telescopes, despite the smaller collecting area of a single ASTRI telescope.inproceedings10.1117/12.30199632024SPIE13095E..0JZ