Next Generation Sky Survey (NGSS)

AO-01-03-OSS-018
The Next Generation Sky Survey
PI: Edward L. Wright, University of California, Los Angeles

The Next Generation Sky Survey (NGSS) will map the entire sky with unprecedented sensitivity from 3.5 to 23 microns. With over 500,000 times the sensitivity of COBE at 3.5 and 4.7 microns, and a thousand times that of IRAS at 12 and 25 microns, NGSS will establish an essential database for testing theories of the origins of planets, stars and galaxies, and is the necessary precursor for NGST. The science objectives of NGSS include finding the most luminous galaxies in the universe, and the closest stars to the sun. NGSS will achieve these dramatic advances while minimizing mission cost and risk by using flight-proven technology for its spacecraft bus components and cryogenic instrument, as well as 2MASS data processing software.

Ames, Harry O. TR Utah State University
Blain, Andrew CoI California Institute of Technology
Cohen, Martin CoI Vanguard Research, Inc.
Cutri, Roc M. CoI California Institute of Technology
Eisenhardt, Peter R. CoI Jet Propulsion Laboratory
Fischer, David TR Ball Aerospace & Technologies Corp.
Gautier, Thomas N. CoI Jet Propulsion Laboratory
Hawkins, Isabel CoI University of California, Berkeley
Jarrett, Thomas H. CoI California Institute of Technology
Kirkpatrick, J. Davy CoI IPAC/Caltech
Lonsdale, Carol J. CoI California Institute of Technology
Mather, John C. CoI NASA/Goddard Space Flight Center
McLean, Ian S. CoI University of California, Los Angeles
McMillan, Robert CoI University of Arizona
Muzilla, Mark TR DRS
Padgett, Deborah L. CoI Jet Propulsion Laboratory
Ressler, Michael E. CoI Jet Propulsion Laboratory
Skrutskie, Michael CoI University of Massachusetts, Amherst
Stanford, S. Adam CoI Lawrence Livermore National Laboratory
Steidel, Charles C. CoI California Institute of Technology
Walker, Russell G. CoI Vanguard Research, Inc.
Wright, Edward L. PI University of California, Los Angeles


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NASA Headquarters Responsible Office: Code SZ
Last Updated: 11 May 2002
Author: Paul Hertz (Code SZ)