Multi-Messenger Astronomy with Extremely Large Telescopes
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.
- Publication:
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Bulletin of the American Astronomical Society
- Pub Date:
- May 2019
- DOI:
- arXiv:
- arXiv:1903.04629
- Bibcode:
- 2019BAAS...51c.237C
- Keywords:
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- Astrophysics - High Energy Astrophysical Phenomena;
- Astrophysics - Cosmology and Nongalactic Astrophysics;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- White paper submitted to the Astro2020 Decadal Survey