2017/08/21 by W. Guerin, A. Dussaux, M. Fouché +5 · 1 citation
Physics and Astronomy · #astro-ph.IM #physics.optics #quant-ph
paper · pdf · doi:10.1093/mnras/stx2143
published as MNRAS 472, 4126-4132 (2017) · Accepted for publication in Mon. Not. Roy. Astron. Soc
arxiv created 2017/08/21 · arxiv updated 2018/08/14
We report the first intensity correlation measured with star light since Hanbury Brown and Twiss' historical experiments. The photon bunching g(2)(τ, r=0), obtained in the photon counting regime, was measured for 3 bright stars, α Boo, α CMi, and β Gem. The light was collected at the focal plane of a 1~m optical telescope, was transported by a multi-mode optical fiber, split into two avalanche photodiodes and digitally correlated in real-time. For total exposure times of a few hours, we obtained contrast values around 2×10-3, in agreement with the expectation for chaotic sources, given the optical and electronic bandwidths of our setup. Comparing our results with the measurement of Hanbury Brown et al. on α CMi, we argue for the timely opportunity to extend our experiments to measuring the spatial correlation function over existing and/or foreseen arrays of optical telescopes diluted over several kilometers. This would enable μas long-baseline interferometry in the optical, especially in the visible wavelengths with a limiting magnitude of 10.