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Contents
VLA Expansion Project: June 1998 Design Review
(revised February 1999)
Contents
INTRODUCTION
TECHNICAL OVERVIEW
Primary Goals for the
Components of the Upgrade
The Ultra-Sensitive Array
The A+ Configuration
Antenna and Receiver Improvements
Improved Low Noise Receivers
New Observing Bands at the Cassegrain Focus
New Prime Focus Systems
Sensitivity Goals
A New LO/IF Transmission System
A New Correlator
Improved Surface-Brightness Sensitivity
High Angular Resolution--The A+ Configuration
Example imaging with the A+ configuration
On-Line Computing
Other Capabilities
NEW SCIENCE WITH THE ENHANCED VLA
Imaging-Spectroscopy of Solar Radio Bursts
Bistatic Radar Observations of Planets and Minor Bodies
High-resolution Imaging of Thermal Emission
Imaging Protoplanetary Disks
Transient Phenomena
Extragalactic Surveys
Clusters of Galaxies
Objects at High Redshift
IMPACT ON SCIENCE WITH THE VLBA
Improved Image Quality
Closing the Coverage Gap
Extended Scaled-Array Capability
Snapshot Mode
Synergy
BUDGET AND SCHEDULE
SUMMATION
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VLA Expansion Project Home Page
Michael Rupen
Fri Mar 26 15:30:00 MST 1999