'Ray spectra' diaporamas de présentation

X-Ray Technology

X-Ray Technology. By: PROF. Dr. Moustafa Moustafa Mohamed Faculty of Allied Medical Science Pharos University in Alexandria. Introduction to Medical Imaging. NON Invasive. Uses of medical imaging Obtain information about internal body

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Narrow-Line Seyfert 1 Galaxies Observational and Theoretical Progress until 2003 The Review

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THE PERIODIC TABLE & ELECTRON CONFIGURATION

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Experience in using 3 MeV protons for PIXE application on environmental and biological samples

Experience in using 3 MeV protons for PIXE application on environmental and biological samples. Ana Pantelica, Constantin Ciortea, Marin Marius Gugiu, Daniela Fluerasu, Dana Elena Dumitriu, Dan Gabriel Ghita, Catalin-Ionut Calinescu

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L. Labate, C.A. Cecchetti, M. Galimberti, A. Giulietti, D. Giulietti, L.A. Gizzi, P. Tomassini

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Radio-quiet Isolated Neutron Stars (RQINs)

Radio-quiet Isolated Neutron Stars (RQINs). Jeng-Lwen, Chiu Institute of Astronomy, NTHU 2004/09/30. Outline. Neutron stars AXPs & SGRs CCOs XDINs (with RX J1856.5-3754) Comparison Others Future work. Neutron stars. Introduction. INS = Isolated (non-binary) Neutron Stars

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Obscured and unobscured growth of Super-massive Black Holes

Obscured and unobscured growth of Super-massive Black Holes. Francisco J. Carrera, X. Barcons, J. Bussons, J. Ebrero, M. Ceballos, A. Corral (IFCA, CSIC-UC, Spain) & XMM-Newton Survey Science Centre (S. Mateos, M. J. Page, M.G. Watson, J. Tedds, R. Della Ceca ...).

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The n_TOF Collaboration , cern.ch/nTOF

The n_TOF Collaboration , www.cern.ch/nTOF. Summary of n_TOF measurements performed in 2012 (CERN 44 th INTC meeting, June 26 th 2013). Carlos GUERRERO (CERN Fellow ) n_TOF Run and Analysis Coordinator. n_TOF measurements in 2012. Basic Nucl . P hys. Nuclear technologies.

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Atomic Spectra

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Obscured and unobscured growth of Super-massive Black Holes from the XMM-Newton Medium Survey

Obscured and unobscured growth of Super-massive Black Holes from the XMM-Newton Medium Survey. Francisco J. Carrera, X. Barcons, J. Bussons, J. Ebrero, M. Ceballos, A. Corral (IFCA, CSIC-UC, Spain) and many SSC colleagues. SSC#20, Potsdam, Nov. 13, 2006. NGC4291.

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Survey of Micro Quasars

Survey of Micro Quasars. Outline. Reminder: what is a microquasar? Established and Candidate microquasars Gamma ray candidates: LSI +615, LS 5039 As seen in DC2 Models for gamma ray spectra. What and Where. High Mass XRB live near galactic plane Low Mass XRB live in the bulge.

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Authors:Alexander reporter:???

X-ray spectral constraints for z~2 massive galaxies : the identification of reflection-dominated active galactic nuclei. Authors:Alexander reporter:???. Outline. Introduction Data and stacking procedures Analyses and results Summary. Introduction.

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New insights into optically elusive AGN

New insights into optically elusive AGN. Estelle PONS Mike WATSON. University of Leicester, UK X-ray and Observational Astronomy (XROA) Group. Outline. Introduction Narrow emission-line galaxy sample Selection Classification X-ray & optical properties

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Pgs.

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Potential Neutrino Signals from Galactic ? -Ray Sources

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X-ray Spectroscopy of Laboratory and Astrophysical Plasmas

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Trends in the Chandra X-Ray Spectra of O and Early B Stars

Trends in the Chandra X-Ray Spectra of O and Early B Stars. June 24, 2008. Spectra of Stars. We know that spectra result from physical processes within stars. They often reflect physical properties of the stars that created them. ex. Optical Spectra. X-Ray Spectra of O and Early B Stars.

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ACCRETION ONTO YOUNG STARS WITH IXO

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X-ray spectra for different mask substrate types and gold thicknesses

X-ray spectra for different mask substrate types and gold thicknesses. J.W. Flanagan XDET Mtg. 2013.10.3. HER. Power incident on face of detector. Power absorbed in 2 mm-deep Si detector. Also assume 1.42 cm of Be in path. L ER. Power incident on face of detector.

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Fermi-LAT Study of Cosmic-Ray Gradient in the Outer Galaxy --- Fermi-LAT view of the 3 rd Quadrant ---

SNR RX J1713-3946. B. HESS. ?. 0. e. e. ?. gas. +. +. +. -. -. -. gas. Fermi-LAT Study of Cosmic-Ray Gradient in the Outer Galaxy --- Fermi-LAT view of the 3 rd Quadrant ---.

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