Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
JPL
California Institute of Technology, Pasadena
Caltech Submillimeter Observatory, Caltech 320-47, Pasadena, CA 91125.
Spitzer Science Center, California Institute of Technology, MC 220-6, Pasadena, CA 91125; Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109.
California Inst. of Technology, Pasadena
Jet Propulsion Lab., USA
California Institute of Technology, Downs Laboratory of Physics 320-47, Pasadena, CA 91125; Jet Propulsion Laboratory 264-767, Pasadena, CA 91109.
California Institute of Technology, Pasadena, CA, US
California Institute of Technology, Pasadena.
Spitzer Science Ctr. / California Institute of Technology, USA
National Aeronautics and Space Administration. Ames Research Center, Moffett Field, CA.
California Institute of Technology, Pasadena, CA
Caltech
Chicago, University, Chicago, Ill.
Caltech Submillimeter Observatory, Pasadena, California
Spitzer Science Center, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125.
Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109; Spitzer Science Center, California Institute of Technology, Pasadena, CA 91125. University, Chicago, IL; California Institute of Technology, Pasadena, CA
Caltech / SSC
CalTech
JPL and Caltech
California Institute of Technology, Pasadena, California
ENRICO FERMI INST., UNIV. OF CHICAGO, CHICAGO, IL 60637
ENRICO FERMI INST., THE UNIV. OF CHICAGO, CHICAGO, IL 60637
California Institute of Technology, Pasadena, CA, USA
Chicago Univ., IL.
(Erratum) Physical and chemical structure of the IC 63 nebula. III. Gas-phase carbon abundance.
1.25 MM observations of luminous infrared galaxies
350 Micron Continuum Imaging of the Orion A Molecular Cloud with the Submillimeter High Angular Resolution Camera
A compact density condensation around L1551-IRS 5: 2.7mm continuum observations with 4" resolution
A heterodyne receiver for the submillimeter wavelength region based on cyclotron resonance in InSb at low temperatures
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