PIRSA:24100095

The VERITAS SII Observatory

Kieda, D. (2024). The VERITAS SII Observatory. Perimeter Institute. https://pirsa.org/24100095

Kieda, Dave. The VERITAS SII Observatory. Perimeter Institute, Oct. 30, 2024, https://pirsa.org/24100095 

          @misc{ pirsa_PIRSA:24100095,
            doi = {10.48660/24100095},
            url = {https://pirsa.org/24100095},
            author = {Kieda, Dave},
            keywords = {Cosmology},
            language = {en},
            title = {The VERITAS SII Observatory},
            publisher = {Perimeter Institute},
            year = {2024},
            month = {oct},
            note = {PIRSA:24100095 see, \url{https://pirsa.org}}
          }

Dave Kieda

University of Utah

Talk number
PIRSA:24100095
Collection
Talk Type
Subject
Abstract
The VERITAS Imaging Atmospheric Cherenkov Telescope array was augmented in 2019 with high-speed focal plane electronics to allow VERITAS for Stellar Intensity Interferometry (VSII) observations. Since December 2019, VSII has been used to measure angular diameters of bright (OBA) stars at an effective wavelength of 416 nm. VSII observations have also served as a testbed to explore hardware and analysis improvements to advance the instrument's sensitivity. VSII has performed more than 730 hours of moonlit observations on 56 bright stars and binary systems ($ -1.46 < m_V < 4.22$). This talk will describe the VSII observatory, highlight selected observations made by the VSII observatory, and describe ongoing improvements in detector instrumentation and analysis.