Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Columbia University
Columbia Astrophysics Lab
Columbia Astrophysics Laboratory
Columbia Astrophysics Laboratory, NY
Columbia Univ., New York, NY.
Danish Space Research Institute, Juliane Maries Vej 30, Copenhagen DK-2100, Denmark, DKColumbia Astrophysics Lab, Columbia University, 136 So. Broadway, Irvington, NY 10533, USA, USCaltech, MC 220-47, Pasadena, CA 91125, USA, USEuropean Synchrotron Radiation Facility, B.P. 200-F, 38043 Grenoble Cedex, France, FR
Columbia Astrophysics Laboratory, Columbia University, New York, NY 10027, USA
Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, USA
Lawrence Livermore National Laboratory, Livermore, CA
Columbia Astrophysics Laboratory, Columbia University, 550 W. 120th Street, NY 10027, New York, USA
LLNL
Columbia Astrophysics Laboratory, Columbia University, New York, NY, USA and; GAPS Collaboration: Columbia University, UC Berkley, UCLA, JAXA / ISAS, Danish Technical University, Oak Ridge National Laboratory, Lawrence Livermore National Laboratory
Columbia University, New York, N.Y.
Columbia
Columbia Astrophysics Lab., USA
Columbia Astrophysics Laboratory, West 120th Street, New York, New York 10025
Lawrence Livermore National Lab.
Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027.
Lawrence Livermore National Laboratory, Livermore, CA, US
Columbia Astrophyisics Lab., USA
Columbia Univ., USA
Columbia Astrophysics Laboratory, 550 West 120th Street, New York, NY 10027
A general purpose calibration facility for use in X-ray astronomy
A hard X-ray spectrometer for high angular resolution observations of cosmic sources.
A high resolution gas scintillation proportional counter for studying low energy cosmic X-ray sources
A large area, low cost, gamma-ray, imaging spectrometer
A new concept for background rejection in gamma-ray astronomy - the supershield
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