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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 3 CONTRIBUTI IN ATTI DI CONVEGNO (Proceedings)
  4. 3.02 Abstract in Atti di convegno
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/32445
Title: ngVLA Key Science Goal 5 Understanding the Formation and Evolution of Black Holes in the Era of Multi-Messenger Astronomy
Authors: Lazio, T. Joseph W.
Alatalo, Katherine
Blecha, Laura
Boizelle, Benjamin
Bower, Geoffrey C.
Braatz, James
Bogdanovic, Tamara
Brisken, Walter
Burke-Spolaor, Sarah
Carbone, Dario
Chomiuk, Laura
Civano, Francesca M.
Comerford, Julia
Condon, James
Coppejans, Deanne
Corsi, Alessandra
Darling, Jeremiah K.
Davis, Timothy A.
Frail, Dale A.
Hall, Kirsten R.
Hallinan, Gregg
Harwood, Jeremy
Kharb, Preeti
Kimball, Amy
Kirkpatrick, Allison
Kording, E. G.
Lacy, Mark
Lazzati, Davide
Lister, Matthew L.
Liu, Xin
Maccarone, Thomas J.
Metzger, Brian
Miller-Jones, J. C. A.
MUKHERJEE, DIPANJAN
Nyland, K. E.
O'Shaughnessy, Richard
Owen, Benjamin
Patil, Pallavi
Pesce, Dominic
Plotkin, Richard M.
PRANDONI, ISABELLA 
Ravi, Vikram
Reid, Mark
Reines, Amy
Rujopakarn, Wiphu
Rupen, Michael P.
Sand, David
Shen, Yue
Simon, Joseph
Sivakoff, Gregory R.
Strader, Jay
Taylor, Greg B.
Taylor, Stephen
van Velzen, Sjoert
Issue Date: 2019
Volume: American Astronomical Society Meeting Abstracts #233
Number: 233
First Page: 361.25
Abstract: The next-generation Very Large Array (ngVLA) will be a powerful telescope for finding and studying black holes across the entire mass range. High-resolution imaging abilities will allow the separation of low-luminosity black holes in the local Universe from background sources, thereby providing critical constraints on the mass function, formation, and growth of black holes. Its combination of sensitivity and angular resolution will provide new constraints on the physics of black hole accretion and jet formation. Combined with facilities across the spectrum and gravitational wave observatories, the ngVLA will provide crucial constraints on the interaction of black holes with their environments, with specific implications for the relationship between evolution of galaxies and the emission of gravitational waves from in-spiraling supermassive black holes and potential implications for stellar mass and intermediate mass black holes. The ngVLA will identify the radio counterparts to transient sources discovered by electromagnetic, gravitational wave, and neutrino observatories, and its high-resolution, fast-mapping capabilities will make it the preferred instrument to pinpoint electromagnetic counterparts to events such as supermassive black hole mergers. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Part of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.
Conference Name: 233 Meeting of American Astronomical Society
Conference Place: Seattle, Washington
Conference Date: 6–10 January, 2019
URI: http://hdl.handle.net/20.500.12386/32445
URL: https://aas.org/meetings/aas233
https://aas.org/sites/default/files/2019-10/aas233_abstracts.pdf
Bibcode ADS: 2019AAS...23336125L
Fulltext: open
Appears in Collections:3.02 Abstract in Atti di convegno

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