Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
UMBC
University of Maryland-Baltimore County, USA
Department of Physics, University of Maryland-Baltimore County
University of Maryland, Baltimore County
GSFC;, University of Maryland, Baltimore County
Department of Astronomy, Boston University, 725 Commonwealth Ave., Boston, Massachusetts 02215
NASA / Goddard Space Flight Center
University of Maryland Baltimore County / GSFC
Department of Physics, University of Maryland Baltimore County, 1000 Hilltop Circle, Baltimore, MD 21250, USA; Astrophysics Science Division, NASA Goddard Space Flight Center, Code 660, Greenbelt, MD 20771, USA
JCA / UMBC
JCA / UMBC, NASA / GSFC
Max-Planck-Institut für Kernphysik, D-69029 Heidelberg, Germany
UMBC / NASA-GSFC
Joint Center for Astrophysics, University of Maryland, Baltimore County, Baltimore, MD, USA
Joint Center for Astrophysics, Physics Department, University of Maryland, Baltimore 1000 Hilltop Circle, Baltimore, MD 21250
Max-Planck-Institut für Kernphysik, Heidelberg, Germany
UMBC / JCA, NASA / GSFC
University of Maryland
UMBC and GSFC
UMBC and Goddard
JCA / UMBC and LHEA / GSFC
Astronomy Dept. Boston University
Department of Astronomy, Boston University
Laboratory for High Energy Astrophysics, NASA Goddard Space Flight Center, Code 661, Greenbelt, MD 20771, USA
University of Maryland Baltimore County
Department of Physics, UMBC, 1000 Hilltop Circle, Baltimore MD 21250; NASA / GSFC, Greenbelt, MD 20771
Department of Physics, University of Maryland, Baltimore County; NASA, Goddard Space Flight Center
Max-Planck-Institut für Kernphysik, Postfach 10 39 80, Heidelberg D 69029, Germany
BOSTON UNIVERSITY
A Chandra Survey of Quasar Jets: Latest Results
A Comprehensive Study Of The Gamma-ray Seds Of The Entire Recalibrated Egret-blazar-database.
A Deep Chandra Observation of the PKS 1055+201 Jets, Lobes, and Hotspots
A Deep Chandra Observation Of The Pks1055+201 Jets, Lobes, And Hotspots
A diagnostic test for determining the location of the GeV emission in powerful blazars
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