PPT-Gamma-ray pulsars discovery by Fermi Space Observatory

Sergei Popov SAI MSU Plan General intro Pulsar models Population synthesis Summary of discoveries EGRET legacy Just 6 pulsars Crab Geminga Vela PSR B105552 PSR B170644 PSR B195132 . Dan Hooper . - . Fermilab. /University of Chicago University of Michigan Dark Matter Workshop, April . 1. 5. . th. , 2013. Dark Matter in The Galactic Center. The volume surrounding the Galactic Center is complex; backgrounds present are not necessarily well understood . 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). Jocelyn Bell . Burnell. University of Oxford Astrophysics . And. Mansfield College. 1957. 2. 3. Crab PSR almost discovered I. Late . summer 1957; . an Open Night . at McDonald; . 82 inch . (Struve) telescope . 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. R. N. Manchester. CSIRO Astronomy and Space Science Australia . Telescope National Facility. , Sydney. Summary. Pulse profiles – doubles and . interpulses. High . Edot. pulsars – radio and high-energy emission. 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 . 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. Jun 22, 2010. HKU Fermi Workshop. Neutron Star Zoo: radio pulsars, . magnetars. , RRATs, CCOs, and more . Special thanks to Vicky . Kaspi. for some materials in this talk . Overview. Since the first pulsar discovered 40 yrs ago, they are . 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. Jocelyn Bell . Burnell. University of Oxford Astrophysics . And. Mansfield College. 1957. 2. 3. Crab PSR almost discovered I. Late . summer 1957; . an Open Night . at McDonald; . 82 inch . (Struve) telescope . 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 (. 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?.