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Science with an ngVLA: The ngVLA Science Case and Associated Science Requirements

Murphy, Eric J. and Bolatto, Alberto and Chatterjee, Shami and Casey, Caitlin M. and Chomiuk, Laura and Dale, Daniel and de Pater, Imke and Dickinson, Mark and Di Francesco, James and Hallinan, Gregg and Isella, Andrea and Kohno, Kotaro and Kulkarni, S. R. and Lang, Cornelia and Lazio, T. Joseph W. and Leroy, Adam K. and Loinard, Laurent and Maccarone, Thomas J. and Matthews, Brenda C. and Osten, Rachel A. and Reid, Mark J. and Riechers, Dominik and Sakai, Nami and Walter, Fabian and Wilner, David (2018) Science with an ngVLA: The ngVLA Science Case and Associated Science Requirements. . (Unpublished) http://resolver.caltech.edu/CaltechAUTHORS:20190403-125128558

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Abstract

The science case and associated science requirements for a next-generation Very Large Array (ngVLA) are described, highlighting the five key science goals developed out of a community-driven vision of the highest scientific priorities in the next decade. Building on the superb cm observing conditions and existing infrastructure of the VLA site in the U.S. Southwest, the ngVLA is envisaged to be an interferometric array with more than 10 times the sensitivity and spatial resolution of the current VLA and ALMA, operating at frequencies spanning ∼1.2−116,GHz with extended baselines reaching across North America. The ngVLA will be optimized for observations at wavelengths between the exquisite performance of ALMA at submm wavelengths, and the future SKA-1 at decimeter to meter wavelengths, thus lending itself to be highly complementary with these facilities. The ngVLA will be the only facility in the world that can tackle a broad range of outstanding scientific questions in modern astronomy by simultaneously delivering the capability to: (1) unveil the formation of Solar System analogues; (2) probe the initial conditions for planetary systems and life with astrochemistry; (3) characterize the assembly, structure, and evolution of galaxies from the first billion years to the present; (4) use pulsars in the Galactic center as fundamental tests of gravity; and (5) understand the formation and evolution of stellar and supermassive blackholes in the era of multi-messenger astronomy.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1810.07524arXivDiscussion Paper
ORCID:
AuthorORCID
Murphy, Eric J.0000-0001-7089-7325
Bolatto, Alberto0000-0002-5480-5686
Casey, Caitlin M.0000-0002-0930-6466
Chomiuk, Laura0000-0002-8400-3705
Dale, Daniel0000-0002-5782-9093
de Pater, Imke0000-0002-4278-3168
Dickinson, Mark0000-0001-5414-5131
Hallinan, Gregg0000-0002-7083-4049
Isella, Andrea0000-0001-8061-2207
Kohno, Kotaro0000-0002-4052-2394
Kulkarni, S. R.0000-0001-5390-8563
Leroy, Adam K.0000-0002-2545-1700
Loinard, Laurent0000-0002-5635-3345
Riechers, Dominik0000-0001-9585-1462
Walter, Fabian0000-0003-4793-7880
Alternate Title:The ngVLA Science Case and Associated Science Requirements
Additional Information:The authors thank the 100’s of community members that have contributed to the definition of the ngVLA science mission and corresponding science requirements. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Part of this work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Funders:
Funding AgencyGrant Number
Associated Universities, Inc.UNSPECIFIED
NASA/JPL/CaltechUNSPECIFIED
Record Number:CaltechAUTHORS:20190403-125128558
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20190403-125128558
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:94408
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:03 Apr 2019 23:15
Last Modified:24 Jul 2019 18:03

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