Presentation + Paper
1 August 2021 Measurement of the second-order g(2) correlation function of visible light from Vega in photon counting mode
Author Affiliations +
Abstract
This paper illustrates the results of an experiment performed in the frame of the Asiago Observatory Stellar Intensity Interferometry program, aimed to exploit the quantum properties of the photon stream emitted from celestial objects. Data are acquired over two telescopes separated by approximately 4 km in photon-counting mode and analyzed in post-processing. The temporal and spatial correlation function g(2) on the bright star Vega has been successfully measured at zero baseline and at a ~2 km baseline. The result is fully consistent with that expected for a source with the angular diameter of Vega (approximately 3.3 mas).
Conference Presentation
© (2021) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michele Fiori, Cesare Barbieri, Luca Zampieri, Giampiero Naletto, and Aleksandr Burtovoi "Measurement of the second-order g(2) correlation function of visible light from Vega in photon counting mode", Proc. SPIE 11835, Quantum Communications and Quantum Imaging XIX, 118350D (1 August 2021); https://doi.org/10.1117/12.2593083
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KEYWORDS
Atmospheric Cherenkov telescopes

Telescopes

Calibration

Stars

Sensors

Correlation function

Photon counting

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