PPT-High Energy Gamma Ray Group

Observing Galactic Center amp Dark Matter Search MAGIC Team Ryoma Murata UT B3 Hiroki Sukeno UT B3 Tomohiro Inada Kobe Univ B3 Fermi Team Yuta Sato TUS B4 Taketo Mimura . ASTROPHYSICAL SCENARIOS. Félix Mirabel. CEA-Saclay-France . *. Neutron stars & Black . holes. in . stellar. . binary. . systems. . that. . radiate. in gamma-rays.. (Will not . refer. 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. High Energy & Cosmic Ray Research Ctr.. North Bengal University. TeV Neutrinos and Gamma rays from Pulsars/Magnetars. Introduction. The energy spectrum of cosmic rays extends to extremely high energies, values exceeding 10. 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. -. What Fermi Adds to the Picture. Brian R. Dennis. GSFC, Solar Physics Lab., Code 671. High Energy Solar . Flares. Eruptive Events. Tutorial on Solar Eruptive Events. Analysis of GBM spectral data. 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. North Bengal University. TeV Neutrinos and Gamma rays from Pulsars/Magnetars. Introduction. The energy spectrum of cosmic rays extends to extremely high energies, values exceeding 10. 20. . eV. .. The origin of the cosmic rays and the mechanism responsible for acceleration of cosmic rays to such high energies . G. amma . R. ays from the Large-scale Disk of the Large . Magellanic. . Cloud. Qing-Wen Tang. 1,2. with Xiang-Yu Wang, . Ruo. -Yu Liu, Fang-Kun Peng and P.H.T. Tam. [1] CCAPP , Ohio State University, USA (with John . Shielding Materials Daniel R. McAlister , Ph.D. PG Research Foundation, Inc. 1955 University Lane Lisle, IL 60532, USA Revision 6 . 1 June 18 , 201 8 Introduction Attenuation or s hielding of gamma r Ileana . Radulescu. , Marian Romeo . Calin. SALMROM . laboratory, Life and Environmental Physics Department,. . Horia Hulubei National Institute for R&D in Physics and Nuclear Engineering (IFIN-HH). Flashes. Gamma Ray . Astronomy. . Beginning. started . as a small budget research program in 1959. monitor. ing. compliance with the 1963 Partial Test Ban Treaty by the Soviet Union, and other nuclear-capable states. T. elescope. Liz Hays. NASA GSFC. Lecture Plan. The Fermi Observatory. Science Motivation. Instruments. Detecting gamma rays with the Large . A. rea Telescope. Instrument Subsystems. Angular resolution. 1. W.Blotz. Motivation. Southern Wide field-of-view Gamma-ray 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?.