Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Princeton
Princeton University
Princeton University & IAS
Princeton & IAS
Princeton Univ. Observ
Department of Astronomy, University of Maryland
Dept. of Astrophysical Sciences, Princeton University
Princeton U., UMD
Princeton U. and U of Maryland
Princeton University Observatory
University of Maryland, College Park
Princeton and Maryland
Institute for Advanced Study; Princeton University Observatory, NJ
Department of Physics, Princeton University, Princeton, NJ 08544, USA
Institute for Advanced Study, Princeton, New Jersey 08540
Princeton Univ., Princeton, NJ, US
Princeton Univ. Observatory, Princeton, NJ, US
Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA
Princeton Univ. Observatory, USA
Princeton Univ., USA
Princeton University, Peyton Hall, Ivy Lane, Princeton, NJ 08544-1001, USA
Institute for Advanced Study, Princeton, NJ 08540, USA
Princeton Univ. Observatory, NJ
Department of Astrophysical Sciences, Princeton University, Princeton NJ 08544, USA
Department of Astrophysical Sciences, Princeton University, Peyton Hall, Princeton, NJ 08544-1001
Department of Astrophysics, Princeton University, New Jersey 08544 dnsatkocab.princeton.edu
Institute for Advanced Study, Princeton, NJ
Department of Physics, Ohio State University, Columbus, OH 43210, USA
Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544
Department of Astrophysical Sciences, Princeton University
Princeton University Observatory, Princeton, New Jersey 08544
Princeton University, NJ
Princeton University Observatory, Princeton, NJ 08544, USA
Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544
Princeton University, Princeton, New Jersey 08544; Institute for Advanced Study, Princeton, New Jersey 08540
Princeton University Observatory; Institute for Advanced Study, NJ
Princeton University, Princeton, NJ 08544
Princeton Uni
A Consistent Microlensing Model for the Galactic Bar
A Gaussian Pupil Coronagraph: A New Approach to Detecting Terrestial Planets
A High Galactic Latitude Dust Template for CMB Polarization Studies
A hydrodynamic approach to cosmology - Texture-seeded cold dark matter and hot dark matter cosmogonies
A Mass-Selected Sample of Galaxy Clusters: Weak Lensing Constraints on the Nature of Dark Energy
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Profile ID: LFWR-SCP-P-12627