Multi-Messenger Astronomy with Extremely Large Telescopes
Multi-Messenger Astronomy with Extremely Large Telescopes
The field of time-domain astrophysics has entered the era of Multi-messenger Astronomy (MMA). One key science goal for the next decade (and beyond) will be to characterize gravitational wave (GW) and neutrino sources using the next generation of Extremely Large Telescopes (ELTs). These studies will have a broad impact across astrophysics, informing our knowledge of the production and enrichment history of the heaviest chemical elements, constrain the dense matter equation of state, provide independent constraints on cosmology, increase our understanding of particle acceleration in shocks and jets, and study the lives of black holes in the universe. Future GW detectors will greatly improve their sensitivity during the coming decade, as will near-infrared telescopes capable of independently finding kilonovae from neutron star mergers. However, the electromagnetic counterparts to high-frequency (LIGO/Virgo band) GW sources will be distant and faint and thus demand ELT capabilities for characterization. ELTs will be important and necessary contributors to an advanced and complete multi-messenger network.
Or Graur、Jennifer Barnes、Tanmoy Laskar、Adam A. Miller、Andrew MacFadyen、Rosalba Perna、Stefano Valenti、Adriano Baldeschi、Dale A. Frail、Dario Carbone、Mansi Kasliwal、Aprajita Hajela、Boris Sbarufatti、Giacomo Terreran、S. Bradley Cenko、Chris Pankow、Thomas Matheson、Yihan Wang、Antonella Palmese、Guy S. Stringfellow、Samaya Nissanke、Edo Berger、Wen-fai Fong、Wolfgang E. Kerzendorf、Sumner Starrfield、Marcelle Soares-Santos、Ben Margalit、Kohta Murase、Melissa Graham、Brian D. Metzger、Mohammad Safarzadeh、J. Craig Wheeler、Christopher P. L. Berry、Gregg Hallinan、Sarah Burke-Spolaor、Ariadna Murguia-Berthier、Joshua S. Bloom、Tarraneh Eftekhari、Kate D. Alexander、Kenta Hotokezaka、Vicky Kalogera、Ryan J. Foley、Eric Bellm、Deanne Coppejans、Locke Patton、Peter K. Blanchard、Federica Bianco、Charles D. Kilpatrick、Paz Beniamini、Daniel M. Siegel、Maria R. Drout、Alessandra Corsi、Daniel Kasen、Niharika Sravan、V. Ashley Villar、Ori Fox、Kerry Paterson、Phillip Macias、Chad Hanna、Dan Milisavljevic、Armin Rest、Adithan Kathirgamaraju、Enrico Ramirez-Ruiz、Lorenzo Sironi、Iair Arcavi、David Radice、Emily Levesque、Maryam Modjaz、Igor Andreoni、Cesar Rojas-Bravo、Eric Burns、Sebastian Gomez、Nathaniel C. Roth、Jonathan Zrake、Jeonghee Rho、Ryan Chornock、Raffaella Margutti、Michael Coughlin、Rachel A. Street、G. Grant Williams、Dimitrios Giannios、David Sand、V. Zach Golkhou、Philip S. Cowperthwaite、Alexander Tchekhovskoy
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Or Graur,Jennifer Barnes,Tanmoy Laskar,Adam A. Miller,Andrew MacFadyen,Rosalba Perna,Stefano Valenti,Adriano Baldeschi,Dale A. Frail,Dario Carbone,Mansi Kasliwal,Aprajita Hajela,Boris Sbarufatti,Giacomo Terreran,S. Bradley Cenko,Chris Pankow,Thomas Matheson,Yihan Wang,Antonella Palmese,Guy S. Stringfellow,Samaya Nissanke,Edo Berger,Wen-fai Fong,Wolfgang E. Kerzendorf,Sumner Starrfield,Marcelle Soares-Santos,Ben Margalit,Kohta Murase,Melissa Graham,Brian D. Metzger,Mohammad Safarzadeh,J. Craig Wheeler,Christopher P. L. Berry,Gregg Hallinan,Sarah Burke-Spolaor,Ariadna Murguia-Berthier,Joshua S. Bloom,Tarraneh Eftekhari,Kate D. Alexander,Kenta Hotokezaka,Vicky Kalogera,Ryan J. Foley,Eric Bellm,Deanne Coppejans,Locke Patton,Peter K. Blanchard,Federica Bianco,Charles D. Kilpatrick,Paz Beniamini,Daniel M. Siegel,Maria R. Drout,Alessandra Corsi,Daniel Kasen,Niharika Sravan,V. Ashley Villar,Ori Fox,Kerry Paterson,Phillip Macias,Chad Hanna,Dan Milisavljevic,Armin Rest,Adithan Kathirgamaraju,Enrico Ramirez-Ruiz,Lorenzo Sironi,Iair Arcavi,David Radice,Emily Levesque,Maryam Modjaz,Igor Andreoni,Cesar Rojas-Bravo,Eric Burns,Sebastian Gomez,Nathaniel C. Roth,Jonathan Zrake,Jeonghee Rho,Ryan Chornock,Raffaella Margutti,Michael Coughlin,Rachel A. Street,G. Grant Williams,Dimitrios Giannios,David Sand,V. Zach Golkhou,Philip S. Cowperthwaite,Alexander Tchekhovskoy.Multi-Messenger Astronomy with Extremely Large Telescopes[EB/OL].(2019-03-11)[2025-05-17].https://arxiv.org/abs/1903.04629.点此复制
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