Xray Beam
X-ray diffraction
Gamma-ray Nova V407 Cyg and Fermi-LAT Galactic Plane Transients Gamma-ray Nova V407 Cyg and Fermi-LAT Galactic Plane Transients C.C. Teddy Cheung (NRC.
Markus B ӧ ttcher Ohio University Athens, OH VHE Gamma-Ray Induced Pair Cascades in Blazars and Radio Galaxies.
Chapter 9. Nuclear Analysis Methods 1.Neutron Activation Analysis 2.Accelerator Mass Spectrometry 3.M ö ssbauer Spectroscopy 4.Ion Beam Analysis.
X-ray Diffraction (XRD) What is X-ray Diffraction Properties and generation of X-ray Bragg’s Law Basics of Crystallography XRD Pattern Powder Diffraction.
Greg Madejski (KIPAC/SLAC) With Masaaki Hayashida, Marek Sikora, Jun Kataoka, Lukasz Stawarz for the Fermi-LAT collaboration Fermi results on AGN: Insights.
Classification of SN Progenitors Optical obs of SNe Classification is relatively straightforward - Spectrum (historically well established) - Luminosity.
Diffuse Gamma Emission of the Galaxy from Cosmic Rays
Geochemical data. All electromagnetic waves travel at the speed of light (3 x 10 8 ms -1 ) and are discussed in terms of wavelength and frequency The.
Galactic Source Populations of VHE Gamma Rays Felix Aharonian Dublin Institute for Advanced Studies, Dublin Max-Planck-Institut f. Kernphysik, Heidelberg.
C. Evoli (SISSA), D. Gaggero (Un. Pisa), D. Grasso (I.N.F.N., Pisa), L. Maccione(SISSA) Diffuse Gamma Emission of the Galaxy from Cosmic Rays.
