PPT-Erich Gamma

Distinguished Engineer VSPlatform ToolsMonaco Surviving Application Scale JavaScript TypeScript in the Trenches 3583 Web based development tools platform and cloud services What do we do. Overview. Key Data. Grant Agreement . n°. 312382. Starting date: 1. st. September 2013. Duration: 48 months (end date 31. st. August 2017). Total Budget: 14.837.981 euro. Consortium Composition. 84 . Hiroshi Nagai. (National Astronomical Observatory of Japan). In collaboration with. Monica . Orienti. , Motoki Kino, Kenta Suzuki, Keiichi Asada, Akihiro . Doi. , Gabriele . Giovannini. , Marcello . Sergei Popov. (SAI MSU). Plan. General intro. Pulsar models. Population synthesis. Summary of discoveries. EGRET legacy. Just 6 pulsars:. Crab. Geminga. Vela. PSR B1055-52. PSR B1706-44 . PSR B1951+32 . (. GammaSIG. ). (. PhysPAG. ). 231. st. AAS. Meeting (2018). Sylvain Guiriec . –. . sguiriec@gwu.edu. Gamma-ray Science Interest Group. (. GammaSIG. ). 2018/01/08. Agenda. PhysPAG. /. GammaSIG. “The e-ASTROGAM mission (exploring the extreme Universe with gamma rays in the MeV-GeV range)”. Enzo . PARADISO. EDUSAFE Final Review. 20 June 2016. Overview. Gamma camera prototype recap. Panoramic gamma Imaging. Gamma sensor calibration. 3-D Gamma imaging. Overview - . 20 June . 2016 . – p. . 1 - ray Imaging Ethan Hull, Matthew Kiser PHDS Corporation, 3011 Amherst Road, Knoxville, TN 37921, USA Historically, radioactive material detection and localization have been accomplished through th catch a burst and notify other observatoriesboth in space and on the ground of its approx-imate locationWithin minutes HETE-2 mayobtain a precise locationCurrent telescopestake much longer to notify o 12/11/20. | . 1. Gamma-rays are ideal probes of a subset of the radioactive isotopes produced in astrophysical transients.. A number of new gamma-ray missions are being developed (ASCENT, COSI, LOX, AMEGO, …) that will improve sensitivities by over an order of magnitude, allowing us to probe more transients and a broader range of isotopes*.. 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). Vikram . Dwarkadas. . (U Chicago). Matthieu. Renaud, . Alexandre. . Marcowith. . (LUPM, U Montpellier). Vincent . Tatischeff. . (. Univ. Paris-. Sud. ). August 11 2017. TevPA 2017 : VVD. 1. We acknowledge support from the FACCTS program at . Founded . March 24, 1937. Founder Dr. Ethel Parker, Beta 1937-39. Lillian Logan, Alpha 1939-42. Ruth Riley, Zeta 1942-44. Noma Dix Winston, Iota 1944-46. Louise Worthington, Beta 1946-48. Ona Bell . Demaree. C. oupling between nucleons and EM field. Electromagnetic and weak interactions can be treated as perturbations. Emission of a . g. -ray is caused by the interaction of the nucleus with an external electromagnetic field. 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?.