PPT-Gamma-Ray astrophysics with current and future detectors

1 WBlotz Motivation Southern Wide fieldofview Gammaray Observatory SWGO Planned to be built to monitor the Southern sky Look for transient phenomena and extended sources What should be the energy range of the observatory. The photomultiplier consists of a photocathode a focusing electrode and 10 or more dynodes that multiply by each electron striking the dynode knocking out more than one electron from every dynode in the chain The anode and dynodes are biased by a ch The UK’s national standards laboratory. World leading . National Measurement Institute . 450+ specialists in . Measurement Science. State-of-the-art laboratory facilities. The heart of the UK’s . Manel. Martinez. 4. 3. rd. . Winter Meeting. March 2015-Benasque. Outline. 1) Introduction. 2) Basics on VHE Gamma Astronomy physics. 3) VHE gamma observatories. 4) CTA. 5. ) Conclusions. 1) INTRODUCTION. Encapsulated Germanium Detectors for Gamma Measurements Features  For compact construction of multi-element detectors for gamma ray applications  For very large efciency and solid angle coverag M87. Studying the Cosmos through..... . Observations. Theory. Experiment. Astro @ Purdue. Astro @ Purdue. 9 . research-active faculty members covering a wide range of topics. Group includes postdoctoral scholars, staff scientists and students. H. . Herrmann (LANL. ). e. -. Next . Steps. Cherenkov detectors . Energy . thresholded. Gas limited to >2.5 . MeV. Solid limited to <~0.2 . MeV. Aerogel. might span the gap. Real . g. -ray spectroscopy (Energy resolved) . Nuclear. . Astrophysics. : first . results. of . tests. and . simulations. of the ELISSA array. Marco La . Cognata. . The 3rd ELIMED Workshop . 7. -10 September . 2016 . Laboratori. . Nazionali. October 1, 2014. Dmitriy Yavid, Broad Shoulder Consulting LLC. Photo detectors have become ubiquitous, amazingly good and dirt cheap. Still, there is an ever-increasing demand from all corners of science and industry. DC-DC Conversion for the CMS Tracker Upgrade. Vertex 2011, Rust, Austria. June 23rd, 2011. Katja Klein. with . L. . Feld, W. Karpinski, . J. . Merz, . O. Scheibling, J. . Sammet, M. Wlochal. 1. . Physik. . DC-DC Conversion for the CMS Tracker Upgrade. Vertex 2011, Rust, Austria. June 23rd, 2011. Katja Klein. with . L. . Feld, W. Karpinski, . J. . Merz, . O. Scheibling, J. . Sammet, M. Wlochal. 1. . Physik. . Michele Punturo. INFN Perugia and EGO. With many slides from Virgo coll. . and ET science team. Italian Embassy. in Tokyo. 1. ELiTES Bilateral Meeting 2013. Why this workshop?. This event has been “catalyzed” thanks to the good willing of Dr. Alberto Mengoni, the Scientific Attaché of the Italian Embassy in Tokyo and it is inserted within the “Italy in Japan - Focus on Science, Technology and Innovation 2013” framework. Liz Hays . (. NASA Goddard Space Flight Center). The Origin of Cosmic Rays. Credit S. . Swordy. Victor Hess and his . “Flight . Ops . Team”, . 1912. From protons. Pion decay. Accelerated protons (p) interact with matter. 1. Julie . McEnery. (NASA/GSFC) on behalf of the AMEGO team.. Active . Galactic . Nuclei. Pulsars. Black Hole Binaries. Sun. Dark Matter. Novae. Gamma-ray Bursts. Diffuse galactic lines. AMEGO Collaboration. Abstract — Thermo - used to measure gamma doses in the medical and environmental surveillance fields. During the past few years, the CEA Reactor Studies Division tested and validated the use of t