Achieving sub-milliarcecond angular resolutions in optical wavelengths with Cherenkov telescopes at ORM
The intensity interferometry technique enables telescopes to achieve exceptionally high angular resolutions, on the order of hundreds of microarcseconds, in the optical range. I will explain how, in contrast to traditional phase interferometry, this technique readily accommodates blue and near UV wavelengths, and is straightforward to expand to
Aula
20 Jun 2024 - 10:00 Europe/London
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