The VERITAS-Stellar Intensity Interferometry (VSII) survey of Stellar Diameters

被引：0
作者：
Kieda, David [1 ]
Davis, Jonathan [1 ,2 ]
LeBohec, Tugdual [1 ]
Lisa, Mike [3 ]
Matthews, Nolan K. [1 ,4 ]
机构：
[1] Univ Utah, Dept Phys & Astron, 115 S 1400 E 201, Salt Lake City, UT 84112 USA
[2] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA
[3] Ohio State Univ, Dept Phys, 174 W 18th Ave, Columbus, OH 43210 USA
[4] Univ Cote Azur, CNRS, INPHYNI, Nice, France
来源：
37TH INTERNATIONAL COSMIC RAY CONFERENCE, ICRC2021 | 2022年
基金：
美国国家科学基金会; 加拿大自然科学与工程研究理事会;
关键词：
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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.
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页数：9
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