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IPFS News Link • Science

Longer Baseline Telescopes Become Possible

08-04-2011 • arclein

The two primary goals for a telescope are sensitivity and angular resolution. Interferometry among telescope arrays has become a standard technique in astronomy, allowing greater resolving power than would be available to a single telescope. In today's IR and optical interferometric arrays, photons arriving at di erent telescopes must be

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Reported By robert klein

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