Intensity Interferometry with Cherenkov Telescopes

Details Intensity Interferometry with Cherenkov Telescopes Intensity Interferometry with Cherenkov Telescopes

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010rmxac..38....5k&link_type=abstract

The Interferometric View on Hot Stars (Eds. Th. Rivinius & M. Curé) Revista Mexicana de Astronomía y Astrofísica (Serie de Confe

Astronomy and Astrophysics

Astronomy

Gamma Rays: Observations, Instrumentation: Interferometers, Stars: Imaging, Techniques: High Angular Resolution, Techniques: Interfereometric

Scientific paper

We discuss the capabilities of Stellar Intensity Interferometry (SII) arrays which can be constructed using next generation of Imaging Air Cherenkov Telescopes (IACTs) arrays. These IACT arrays will have ≈ 100 large diameter (> 8 m) optical reflectors, offering close to 5000 interferometric baselines, ranging from 50 m to more than 1000 m. SII implementation on IACT arrays will enable high resolution ( < 0.1 mas) imaging at short wavebands (B/V bands), which are optimal for study of hot stars.

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