Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
MPE Garching
Max-Planck-Institut fuer Extraterrestrische Physik, Garching, Germany
MPE-Garching
Max-Planck-Intitut fur Extraterrestriche Physik, Garching, Germany
Max-Planck-Institut fuer extraterrestrische Physik, Garching
Max Planck Institut fuer extraterrestrische Physik
MPE
Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany
Max-Planck-Inst. für extraterrestrische Physik, Germany
Max-Planck-Inst. für Physik und Astrophysik, Garching bei München, Germany
Max-Planck-Inst. für extraterrestrische Physik, Garching bei München, Germany
MAX-PLANCK-INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK, Garching bei München, Germany
Max-Planck-Institut fuer extraterrestrische Physik, Garching, Germany;
MPE Garching, Germany
Max Planck Institut fuer Extraterrestrische Physik
MPE, Garching
MPE, Garching, D
MPE Garching;
MPE, Garching, Germany
Institute for Astronomy, University of Hawaii,USA; Istituto di Radioastronomia del CNR, Bologna, Italy; Max-Planck-Institut fuer Extraterrestrische Physik, Garching bei Muenchen, Federal Republic of Germany, Harvard--Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA; Royal Observatory Edinburgh, Edinburgh, United Kingdom
MPE, Garching, DE
MPE, Germany
Max-Planck-Institut für extraterrestrische Physik, Germany
Max-Planck-Institut für Kernphysik, Heidelberg, Germany
Max-Planck-Institut für Physik und Astrophysik, Garching bei München, Germany
NOAA, Aeronomy Laboratory, Boulder, CO; Max-Planck-Institut für Kernphysik, Heidelberg, Germany
Max-Planck-Institut für extraterrestrische Physik, München, Germany
Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 85748 Garching bei München, Germany
Max
A Catalog of Compact Groups of Galaxies in the SDSS Commissioning Data
A Coordinated XMM, SZE and Optical Survey for Galaxy Cluster Cosmology
A Coordinated XMM, SZE and Optical Survey for Galaxy Cluster Cosmology
A detailed Chandra Study of the cluster with the most luminous cooling core at z>0.25
A Dynamical Study of Optically Selected Distant Clusters
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