Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
The PLANET collaboration
The PLANET Collaboration
Perth Observatory;
GSI
the PLANET Collaboration
OGLE, MicroFUN, MOA, PLANET / RoboNET
the EROS collaboration
Department of Physics, University of Strathclyde, 107 Rottenrow, Glasgow G4 0NG, UK
Department of Earth Sciences, University of Cambridge, Downing Street, Cambridge, UK CB2 3EQ United Kingdom Observatory, Edinburgh, Scotland
University of Torino, Dipartimento di Fisica Generale, Torino, Italy
SMT Observatory c.o. Steward Observatory, Tucson, AZ 85721, USA
Royal Greenwich Observatory, Herstmonceux, England
Akademiia Nauk SSSR, Institut Zemnogo Magnetizma, Ionosfery i Rasprostraneniia Radiovoln, Akademgorodok, USSR; Cuban Academy of Sciences, Institute of Geophysics and Astronomy, Cuba
Torino, Università, Turin, Italy
Istituto di Fisica Generale, Università di Torino
Carleton College
Institut d'Astrophysique Spatiale
University of Torino, Torino, Italy
Universite de Pau et des Pays de l'Adour, Universite de Pau et des Pays de l'Adour, CNRS et INRIA Magique-3D, Laboratoire de Modelisation et d'Imagerie en Geosciences UMR 5212, Avenue de l'Universite, Pau, 64013, France de Ciencias de Cuba, Instituto de Geofisica y Astronomia, Havana, Cuba
Turin
Illinois State University, Department of Physics, Normal, IL 61790-4560, USA
Composite Mirror Applications
Perth Observatory, Australia.
Torino, Univ., Turin, Italy
Perth Observatory, Walnut Road, Bickley, 6076, Perth, Australia
Turin Univ., Italy.
Composite Mirror Applications, Inc., 100 Research Loop, Tucson AZ, 85710, USA
Mail Stop 183-501, Jet Propulsion Laboratory, 4800 Oak Grove Dr., Pasadena, CA 91109
CMA, Inc.
Royal Greenwich Observatory, Cambridge, UK
University of Wyoming
Perth Observatory, Murdoch University
Perth Observatory, Bickley, Australia
Busek Company, Inc.
Physics, Illinois State University, Normal, IL, USA;
A Cold Neptune-Mass Planet OGLE-2007-BLG-368Lb: Cold Neptunes Are Common
A Complete Set of Solutions For Caustic-Crossing Binary Microlensing Events
A method for determining the cosmological deceleration parameter Q sub 0
A method for the automatic separation of the images of galaxies and stars from measurements made with the COSMOS machine
A Monte Carlo simulation of the Sudbury Neutrino Observatory proportional counters
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