Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
SSC / Caltech
Spitzer Science Center, Caltech;
Spitzer Science Center, Pasadena, USA
SIRTF
SSC, Caltech
SIRTF Science Center
SIRTF Science Center / Caltech
Caltech, CA
Spitzer Science Center / Caltech
SIRTF Science Center, Caltech
1 Spitzer Science Center; 2 Caltech; 3 Cornell; 4 University of British Columbia; 5 University of Crete
Caltech / SSC
California Institute Of Technology
Spitzer Science Center, California Institute of Technology, MS 220-6, Pasadena, CA 91125, USA
SIRTF Science Ctr. / CALTECH
Caltech
Spitzer Science Center, Caltech MC 220-6, Pasadena, CA 91125, USA
Palomar Observatory, Pasadena, CA, US
Spitzer Science Center Caltech
IPAC
Spitzer Science Center, California Institute of Technology, Pasadena, CA 91125 Science Center, California Institute of Technology, MC 314-6, Pasadena, CA 91125 Science Center, California Institute of Technology, MC 220-6, Pasadena, CA 91125.
Spitzer Science Center, California Institute of Technology, Pasadena, CA 91125.
California Institute of Technology, Pasadena, CA, US
Spitzer Space Science Center, California Institute of Technology, Pasadena, CA 91125, USA
SSC-Caltech
Palomar Observatory, California Institute of Technology, Pasadena, CA, US
University of California, Berkeley, CA, US
SIRTF / SSC
Caltech, SSC
California Institute of Technology, USA
Spitzer Science Center, California Institute of Technology, Mail Code 220-6, 1200 East California Boulevard, Pasadena, CA 91125.
JPL Caltech
CalTech
Spitzer Science Center, MS 220-06, California Institute of Technology, Pasadena, CA, 91125
SSC, Pasadena, CA
Spitzer Science Center, California Institute of Technology
Infrared Processing and Analysis Center
California Inst. of Technology, Pasadena, CA, US
California Institute of Technology, Pasadena, CA.
Caltech / Spitzer
0.05 Arcsec Imaging Polarimetry of the Gravitational Lens F10214+4724
16 micron Imaging around the Hubble Deep Field North with the Spitzer IRS
16 micron Imaging around the Hubble Deep Field North with the Spitzer IRS.
A bridge between ultraluminous and normal galaxies at high redshifts: Spitzer imaging of a unique spectroscopic radio field
A Comparison of Non-interacting Disk Galaxies in Goals and Sings
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