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The top documents tagged [kev fe]
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kev fe
IAP – Atelier Pulsar P. Laurent 16 Janvier 2006 1 SIMBOL-X Simbol-X Un observatoire dastrophysique X dur à lhorizon 2013 0.1–10 keV 15 keV-10 MeV 0.5 -
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Silicon Drift Detectors for Energy Dispersive X- Ray Fluorescence ( SDDEXRF)
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Sd dpresentation13 nov2011
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Experiments in X-Ray Physics Lulu Liu Partner: Pablo Solis Junior Lab 8.13 Lab 1 October 22nd, 2007.
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NEI Modeling What do we have? What do we need? 2012.08.09 AtomDB workshop Hiroya Yamaguchi (CfA) Fe ion population in CIE (AtomDB v.2.0.2) Temperature.
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The Galactic Center is a Treasure Box of High Energy Physics The Nearest AGN and Star Burst Galaxy. I will report a current picture of the Galactic Center,
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On some prospects of the LOFT mission Institute of Physics, Silesian University in Opava Astronomical Institute, Prague Gabriel Török, Pavel Bakala, Vladimír.
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On Some Prospects of the LOFT Mission: QPO Models Institute of Physics, Silesian University in Opava Gabriel Török CZ.1.07/2.3.00/20.0071 Synergy, GAČR.
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The cooling-flow problem
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The diffuse X-ray emission from the Galactic center
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Recent Chandra Observations of The Galactic Center
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On S ome P rospects of the LOFT M ission : QPO Models
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