Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Max-Planck-Institut fuer extraterrestrische Physik, Garching
MPE, Caltech
Max-Planck / Garching
Caltech;
Department of Astronomy, Caltech, MC 105-24, 1200 East California Blvd., Pasadena, CA 91125, USA
California Institute of Technology, MC 105-24, Pasadena, CA 91125, USA
California Institute of Technology, 220-6, Pasadena, CA 91125, USA; Max-Planck institute for Plasma Physics & Excellence Cluster Boltzmans strasse 2, Garching 86748, Germany
IPP
California Institute of Technology
Caltech
MPE, Garching
Excellence Cluster Universe / IPP, Garching
Max-Planck Institut fuer Extraterrestrische Physik
Max-Planck-Institute for Plasma Physics, Garching
IPP Garching
Caltech / SSC
Max-Planck Institut fuer extraterrestrische Physik
Max-Planck-Institut fuer extraterrestrische Physik, Garching b. Muenchen;
Univ. di Salerno & INFM, Italy
CIT
Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany & Caltech, Pasadena, California, USA
Department of Astronomy, MS 105-24, California Institute of Technology, Pasadena, CA 91125, USA
Astrophysikalisches Institute Potsdam Germany
MPIPP, Germany
Department of Astronomy, California Institute of Technology, Pasadena, CA 91125, USA; Max Planck Institute for Plasma Physics and Cluster of Excellence, Garching bei München, Germany
MPE, Germany
Max Planck Institute for Plasma Physics, Germany
Max-Planck-Institut für Astronomie, Germany
Astrophysikalisches Institut Potsdam, Sternwarte Babelsberg, An der Sternwarte 16, D-14482 Potsdam, Germany
California Institute of Technology, MC 105-24, 1200 East California Boulevard, Pasadena, CA 91125, USA
(U)LIRG Morphology and Color: 70 μm Selected Galaxies in the COSMOS Field
A candidate tidal disruption event in the Galaxy cluster Abell 3571
A Far-IR Characterization of 24 micron Selected Galaxies at 0<z<2.5 using Stacking at 70 microns and 160 microns in the COSMOS Field
A Herschel view of the far-infrared properties of submillimetre galaxies
A Large Sample Of z>3.5 Galaxies With Keck Deimos Spectroscopy
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