PPT-The Fermi Gamma-ray Space

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. for the 1. st. Advanced LIGO Science Run. Jordan Camp. NASA Goddard Space Flight Center. Moriond. Gravitation Meeting. March 25, 2015. Search Team. Lindy Blackburn (. CfA. ). Nelson Christensen (Carleton College). 84 . Hiroshi Nagai. (National Astronomical Observatory of Japan). In collaboration with. Monica . Orienti. , Motoki Kino, Kenta Suzuki, Keiichi Asada, Akihiro . Doi. , Gabriele . Giovannini. , Marcello . 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. Radiation-Dominated Jet?. Kunihito. . Ioka. (KEK). T. Inoue, Asano & KI, . arXiv. : 1011.6350. KI. , . arXiv. : 1006.3073. Suwa. & KI, . arXiv. : 1009.6001. KI+, in . preparation (. 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 . David Smith. Centre d’Etudes Nucléaires de Bordeaux-Gradignan. ( CENBG - in2p3 - CNRS ). I. nstitut. de Physique Nucléaire de Lyon. 6 mars 2015. Le ciel en rayons gamma. avec le. . satellite . Fermi . from Supernova Remnants . to Pulsar Wind Nebulae. Stephen C.-Y. Ng. McGill University. Special thanks to Pat . Slane. for. some materials in this talk . Jun 21, 2010. HKU Fermi Workshop. Outline. SNRs and . Probes and Rovers. Definitions. Satellite – object that revolves around another object in space. Natural – the moon. Man-Made. Telescope – device built to observe distant objects by making them appear closer. . for. New . Stellar. . Sources. of Gamma-. R. ays. Josep Martí. Escuela Politécnica Superior de Jaén. Universidad de Jaén (UJA). Spain. Search. . for. New . Stellar. . S. ources. of Gamma-. 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. 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 . Francesco Loparco*. Salvatore De Gaetano, Mario Nicola . Mazziotta. . on behalf of the Fermi LAT Collaboration. *e-mail: francesco.loparco@ba.infn.it. The gamma-ray Moon. 1. The Moon is among the brightest sources in the gamma-ray sky. Observing Galactic Center & . 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 (. 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?.