DSN Radio Astronomy
Capability Development

Last updated by Tom Kuiper on 1999 May 11

The limited resources of the TMO Radio Astronomy program are focused developing capabilities with high scientific interest which build on particular strengths of the DSN. This document presents the technical goals at a high level. From these, detailed capability goals have been derived.

Investigators and potential investigators are invited to comment on these goals and the priority which should be assigned to them by sending e-mail to Tom Kuiper and posting their views on the DSN Radio Astronomy Discussion Forum.

Capability Science Area JPL & DSN Assets Tasks and Challenges Status
mm-wave VLBI quasars, galactic nuclei 34-m antennas around the world pointing,
aperture correction,
solid outer panels,
one mm-capable 34-m per DSN site
85-105 GHz receiver being tested on DSS-13
mm-wave spectroscopy star formation, many others 34-m antennas in both N & S hemispheres
magnetic field strength measurements star formation long-term development environment control of systematic errors 33 GHz system being checked out at DSS-13
broadband (>250 MHz) spectroscopy evolution of galaxies large antennas demonstrate downconverter performance 300/500 MHz 1024-ch spectrometer ready for testing
broadband RF pre-selector filter ready for testing
spectral line surveys interstellar chemistry,
origin of biochemistry
WBSA, CSP develop automatic data acquisition and analysis software potential; no current development

These development activities are listed in some rough order of priority, with the following rationale:

The following currently authorized or proposed projects are involved in or will benefit from the development activities.

Millimeter wavelength Space VLBI ARISE
Millimeter wavelength VLBI (CMVA)
Search for CO Emission from High-Z Galaxies Seiffert
Search for Circumnuclear Water Masers Greenhill
Monitoring Extragalactic Water Masers Whiteoak
Search for Complex Organic Molecules Levin
Zeeman Measurements of Magnetic Fields in Dark Clouds Levin
Spectral Imaging of Star Formation Langer