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Multi-Messenger Astronomy with Extremely Large Telescopes

Published onMay 31, 2019
Multi-Messenger Astronomy with Extremely Large Telescopes
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Abstract

A key goal for Multi-Messenger Astronomy will be to characterize gravitational wave and neutrino sources using the next generation of Extremely Large Telescopes. These studies will have a broad impact across astrophysics. The counterparts to high-frequency GW sources will be distant and faint and thus demand ELT capabilities for characterization.

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