Optical intensity interferometry lab tests in preparation of stellar diameter measurements at IACTs at GHz photon rates

Abstract

Astronomical intensity interferometry enables quantitative measurements of the source geometry by measuring the photon fluxes in individual telescopes and correlating them, rather than correlating the electromagnetic waves' amplitudes. This simplifies realization of large telescope baselines and high angular resolutions. Imaging Atmospheric Cherenkov Telescopes (IACTs), intended to detect the optical emission of $\gamma$-ray induced air showers, are excellent candidates to perform intensity correlations in the optical at reasonable signal-to-noise ratios. The detected coherence time is on the scale of $10^{-12}$ to $10^{-15}$~seconds - depending on the optical bandwidth of the measurement - which challenges the detection system to work in a stable and accurate way. We developed an intensity interferometry setup applicable to IACTs, which measures the photo currents from photomultipliers and correlates them offline, and as such is designed to handle the very large photon rates provided by the telescopes. We present measurements in the lab simulating starlight using a xenon lamp and measured at different degrees of temporal and spatial coherence. Necessary calibration procedures are described with the goal of understanding the measurements quantitatively. Measured coherence times between $5$femtoseconds (corresponding signal-to-background ratio $5\cdot 10^{-7}$) and $110$femtoseconds (signal-to-background ratio $10^{-5}$) are in good agreement with expectations, and so are the noise levels in the correlations, reaching down to $6\cdot 10^{-8}$, after measurements between $30$minutes and $1$ hour.

References in corpus (10)

• First Results from the CHARA Array. II. A Description of the Instrument
• Optical Interferometry in Astronomy
• The optical system of the H.E.S.S. imaging atmospheric Cherenkov telescopes, Part I: layout and components of the system
• Optical Intensity Interferometry with the Cherenkov Telescope Array
• Demonstration of stellar intensity interferometry with the four VERITAS telescopes
• Optical intensity interferometry observations using the MAGIC imaging atmospheric Cherenkov telescopes
• A quantitative comparison of amplitude versus intensity interferometry for astronomy
• Intensity Interferometry with Aqueye+ and Iqueye in Asiago
• Optical long baseline intensity interferometry: prospects for stellar physics
• Intensity interferometry: Optical imaging with kilometer baselines

Cited by in corpus (3)

• First Intensity Interferometry Measurements with the H.E.S.S. Telescopes
• Comparing Different Approaches for Stellar Intensity Interferometry
• Simultaneous Two Colour Intensity Interferometry with H.E.S.S