Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Pennsylvania State University
Stanford
Laboratory for Computational Astrophysics at the National Center for Supercomputing Applications
KIPAC, Stanford
Stanford University
Max Planck Institute
Center for Astrophysics at Harvard University
KIPAC, Stanford University
Penn State University
CFA
CfA
Penn State
Kipac / Stanford
KIPAC / Stanford
KIPAC, Stanford; Kitp, Ucsb
Stanford / KIPAC
Kavli Institute for Particle Astrophysics and Cosmology / SLAC
Harvard
Max Planck Institut fuer Astrophysik, Garching
Harvard Univ.
Laboratory for Computational Astrophysics, NCSA, University of Illinois at Urbana / Champaign
Harvard Smithsonian Center for Astrophysics
KIPAC / Stanford / SLAC
Dept. of Phys. and Kavli Inst., Stanford University
NCSA / MPA
CfA, IoA
Harvard, CfA
CfA, Harvard
Laboratory for Computational Astrophysics, University of Illinois at Urbana, Urbana, IL;
MPI Garching
Penn State U.
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85748 Garching bei München, Germany; Joint Institute for Laboratory Astrophysics, Campus Box 440, Boulder, CO
KIPAC Stanford
Penn State University, University Park, PA, USA
KIPAC, Stanford University, Menlo Park, California, USA
KIPAC, Stanford University, 2575 Sand Hill Rd., Menlo Park, CA, 94025
KIPAC, Stanford University, 2575 Sand Hill Road, Menlo Park, CA 94025, USA
Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Menlo Park, CA 94025
Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 2575 Sand Hill Road, Menlo Park, CA 94025, USA
Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305
KIPAC / Stanford, CA 94305
Department Astronomy & Astrophysics Pennsylvania State University
Department of Astronomy & Astrophysics, Pennsylvania State Univer
A Grid Based Method for the Radiation Transfer from Multiple Point Sources in the Late Redshift Universe
A Minihalo Model for the Lyman Limit Absorption Systems at High Redshift
A Multi-Code Analysis Toolkit for Astrophysical Simulation Data
A new view of the dwarf spheroidal satellites of the Milky Way from VLT/FLAMES: Where are the very metal poor stars?
Absorption Line Signatures of Delayed Dwarfs
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