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

Zmija A, Vogel N, Anton G, Malyshev D, Michel T, Zink A, Funk S (2022)


Publication Type: Journal article

Publication year: 2022

Journal

Book Volume: 509

Pages Range: 3113-3118

Journal Issue: 3

DOI: 10.1093/mnras/stab3058

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 the realization of large telescope baselines and high angular resolutions. Imaging Atmospheric Cherenkov Telescopes (IACTs), intended to detect the optical emission of γ-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)-(10-15) s-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 set-up applicable to IACTs, which measures the photocurrents 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 × 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 × 10-8, after measurements between 30 min and 1 h.

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How to cite

APA:

Zmija, A., Vogel, N., Anton, G., Malyshev, D., Michel, T., Zink, A., & Funk, S. (2022). Optical intensity interferometry lab tests in preparation of stellar diameter measurements at IACTs at GHz photon rates. Monthly Notices of the Royal Astronomical Society, 509(3), 3113-3118. https://doi.org/10.1093/mnras/stab3058

MLA:

Zmija, Andreas, et al. "Optical intensity interferometry lab tests in preparation of stellar diameter measurements at IACTs at GHz photon rates." Monthly Notices of the Royal Astronomical Society 509.3 (2022): 3113-3118.

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