Multi-Messenger Astronomy with Extremely Large Telescopes
by Ryan Chornock, Philip S. Cowperthwaite, Raffaella Margutti, Dan Milisavljevic, Kate D. Alexander, Igor Andreoni, Iair Arcavi, Adriano Baldeschi, Jennifer Barnes, Eric Bellm, Paz Beniamini, Edo Berger, Christopher P. L. Berry, Federica Bianco, Peter Blanchard, Joshua S. Bloom, Sarah Burke-Spolaor, Eric Burns, Dario Carbone, S. Brad Cenko, Deanne Coppejans, Alessandra Corsi, Michael Coughlin, Maria Drout, Tarraneh Eftekhari, Ryan J. Foley, Wen-fai Fong, Ori Fox, Dale A. Frail, Dimitrios Giannios, V. Zach Golkhou, Sebastian Gomez, Melissa Graham, Or Graur, Aprajita Hajela, Gregg Hallinan, Chad Hanna, Kenta Hotokezaka, Vicky Kalogera, Daniel Kasen, Mansi Kasliwal, Adithan Kathirgamaraju, Wolfgang E. Kerzendorf, Charles D. Kilpatrick, Tanmoy Laskar, Emily Levesque, Andrew MacFadyen, Phillip Macias, Ben Margalit, Thomas Matheson, Brian D. Metzger, Adam A. Miller, Maryam Modjaz, Kohta Murase, Ariadna Murguia, Samaya Nissanke, Antonella Palmese, Chris Pankow, Kerry Paterson, Locke Patton, Rosalba Perna, David Radice, Enrico Ramirez-Ruiz, Armin Rest, Jeonghee Rho, Cesar Rojas-Bravo, Nathaniel C. Roth, Mohammad Safarzadeh, David Sand, Boris Sbarufatti, Daniel M. Siegel, Lorenzo Sironi, Marcelle Soares-Santos, Niharika Sravan, Sumner Starrfield, Rachel A. Street, Guy S. Stringfellow, Sasha Tchekhovskoy, Giacomo Terreran, Stefano Valenti, V. Ashley Villar, Yihan Wang, J. Craig Wheeler, G. Grant Williams, and Jonathan Zrake
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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