Paper
28 July 2008 Toward a revival of stellar intensity interferometry
Author Affiliations +
Abstract
Building on technological developments over the last 35 years, intensity interferometry now appears a feasible option by which to achieve diffraction-limited imaging over a square-kilometer synthetic aperture. Upcoming Atmospheric Cherenkov Telescope projects will consist of up to 100 telescopes, each with ~100m2 of light gathering area, and distributed over ~1km2. These large facilities will offer thousands of baselines from 50m to more than 1km and an unprecedented (u,v) plane coverage. The revival of interest in Intensity Interferometry has recently led to the formation of a IAU working group. Here we report on various ongoing efforts towards implementing modern Stellar Intensity Interferometry.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stephan LeBohec, Cesare Barbieri, Willem-Jan de Wit, Dainis Dravins, Philippe Feautrier, Cédric Foellmi, Andreas Glindemann, Jeter Hall, Jamie Holder, Richard Holmes, Pierre Kervella, David Kieda, Etienne Le Coarer, Stephan Lipson, Fabien Malbet, Sébastien Morel, Paul Nuñez, Aviv Ofir, Erez Ribak, Swapan Saha, Markus Schoeller, Boriz Zhilyaev, and Hans Zinnecker "Toward a revival of stellar intensity interferometry", Proc. SPIE 7013, Optical and Infrared Interferometry, 70132E (28 July 2008); https://doi.org/10.1117/12.787443
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CITATIONS
Cited by 11 scholarly publications.
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KEYWORDS
Atmospheric Cherenkov telescopes

Telescopes

Interferometry

Stars

Interferometers

Optical correlators

Receivers

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