  The VERITAS Imaging Air Cherenkov Telescope (IACT) array was augmented in
2019 with high-speed focal plane electronics to allow its use for Stellar
Intensity Interferometry (SII) observations. Since January 2019, the VERITAS
Stellar Interferometer (VSII) recorded more than 250 hours of moonlit
observations on 39 different bright stars and binary systems ($m_V < 3.74$) at
an effective optical wavelength of 416 nm. These observations resulted in the
measurement of the diameters of several stars with better than 5% resolution.
This talk will describe the status of the VSII survey and analysis.
