Mathematics – Optimization and Control
Scientist
Mathematics
Optimization and Control
Scientist
TRW, Inc., USA
SAMPLE Collaboration
STScI
Cornell University, 404 Space Sciences Bldg., Ithaca, NY 14853-6801
Commissariat a l'Energie Atomique
Louisiana State University, Baton Rouge, La.
Department of Physics, University of York, Heslington, York, UK
Jet Propulsion Lab., California Institute of Technology, Pasadena, CA.
SETI Institute
Los Alamos National Laboratory, Los Alamos, New Mexico 87545
SETI Institute, 515 N. WHisman Road, Mountain View, CA 94043, USA
Cornell Univ., Ithaca, NY, US
Space Sciences Building, Cornell University, Ithaca, New York
Center for Radiophysics and Space Research, Cornell University, Ithaca, New York
Paris, Observatoire, Meudon, France; Cornell University, Ithaca, NY
NASA Ames Research Center, Moffett Field, CA; SETI Institute, Mountain View, CA
Los Alamos National Lab.
Los Alamos National Lab., NM
SETI Institute, 2035 Landings Drive, Mountain View, CA 94043, USA
SETI Institute, NASA Ames Research Center, Moffett Field, California
M / S 245-3, NASA Ames Research Center, Moffett Field, California
NASA Ames Research Center
Cornell University, Ithaca, NY, US
Mars Institute, SETI Institute, NASA Ames Research Center
SETI Institute, NASA Ames Research Center, Moffett Field, CA 94035-1000, USA
NASA Ames Research Center, Moffett Field, CA, USA
Cornell Univ., Ithaca, NY.
Department of Astronomy, Cornell University, Ithaca, New York
Mars Institute, SETI Institute, and NASA Ames Research Center, Moffett Field, CA 94035-1000, USA
Mars Institute, SETI Institute, and NASA Ames Research Center, MS 245-3, Moffett Field, CA 94035, USA
SETI Institute, USA
Mars Institute, USA and SETI Institute, USA and NASA Ames Research Ctr., USA
183 GHz InP MMIC Based Radiometer
40 CCDs of the MegaCam wide-field camera: procurement, testing, and first laboratory results
A case study of impact-induced hydrothermal activity: The Haughton impact structure, Devon Island, Canadian High Arctic
A fine analysis of the helium-rich star HD 184927.
A Method for Increasing the Dynamic Response of Photometric Systems
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