Next-generation facility · Proposed
Next Generation Very Large Array
A proposed radio interferometer, designed as the successor to the Very Large Array and a complement to ALMA, that would observe the centimetre-to-millimetre sky with far greater sensitivity and resolution — imaging planet-forming discs, molecular gas, and the distant universe. Led by the U.S. National Radio Astronomy Observatory.
Facilities, methods & instruments
Knowledge connections
- Associated withVery Large Array
- Associated withNational Radio Astronomy Observatory
- Associated withRadio Interferometry
- Associated withAperture Synthesis
- Associated withRadio
- Associated withMillimeter
Sources
The primary and reference sources this topic draws on.
- NSF NOIRLabNSF National Optical-Infrared Astronomy Research Laboratory
Ground-based optical/infrared observatory data and imagery.