High energy astrophysics - PowerPoint PPT Presentation

Sorin ZGURA E -Mail: szgura@spacescience.ro spacescience.ro

Sorin ZGURA E -Mail: szgura@spacescience.ro http:// www.spacescience.ro. What is ISS?. INSTITUTE OF SPACE SCIENCE legal subsidiary of the National Institute for Laser, Plasma and Radiation Physics (INFLPR). (http:// www.spacescience.ro ). What is ISS history?.

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Introduction and Overview

Introduction and Overview. X-ray/Gamma-ray Astronomy. The Great Observatories. Chandra. High Energy Astrophysics Sample Sources Professor George F. Smoot Extreme Universe Lab, SINP Moscow State University. Great Observatories. Opacity of Atmosphere. Versus characteristic temperature.

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Astroparticle Physics: Puzzles and Discoveries

Astroparticle Physics: Puzzles and Discoveries. V. Berezinsky Laboratori Nazionali del Gran Sasso, INFN Sendai, Japan September 11, 2007. Formula of astrophysical discoveries:. ALL GREATEST DISCOVERIES IN ASTROPHYSICS APPEARED UNPREDICTABLY AS PUZZLES. WHAT WAS PREDICTED WAS NOT DISCOVERED.

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Active Galactic Nuclei

Active Galactic Nuclei. 4C15 - High Energy Astrophysics jlc@mssl.ucl.ac.uk http://www.mssl.ucl.ac.uk/. 6. Active Galactic Nuclei (AGN): AGN accretion; Sources of energy; Radio galaxies and jets; [2]. Introduction. Apparently stellar Non-thermal spectra High redshifts

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Astronomy 12 Stars, Stellar Evolution, and High Energy Astrophysics

Astronomy 12 Stars, Stellar Evolution, and High Energy Astrophysics - Stan Woosley The Nature of Astronomy The study of objects beyond earth (here with emphasis on stars and physics)

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The International Astronomical Union Programs for supporting the teaching of astronomy

The International Astronomical Union Programs for supporting the teaching of astronomy in developing countries Thailand and Laos January 2007 John Hearnshaw University of Canterbury, New Zealand Chair of IAU Comm. 46 Program Group for the Worldwide Development of Astronomy.

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The Future of High Energy Astrophysics group in Ond řejov

The Future of High Energy Astrophysics group in Ond řejov. 3rd INTEGRAL/BART Workshop Nov 3, 2004. The HEA Group in Ondrejov. 14 staff members (some part-time) , mostly scientific , 6 PhD 3 PhD students (Majlo, Torman, Toast) 1 Diploma student (Lado)

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Potential Italian contributions to WFI

Potential Italian contributions to WFI. L. Piro, IAPS-Rome on behalf of the Athena Italian team. The rationale. T he primary Italian contribution to mission elements is XIFU O ther smaller contributions include participation to mirror and Ground Segment activities.

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X-ray Polarimeter

Biswajit Paul Raman Research Institute, Bangalore. X-ray Polarimeter. X-ray Polarimeter Team at RRI. Biswajit , Rishin , Gopala Krishna, Duraichelvan , Chandreyee , Ateequlla , Arasi , Jincy , Mamatha , Marykutty , Nagaraj , Rajagopal , Sandhya , …. Measurement Technique

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Marshall Space Flight Center Launching the Future of Exploration and Science

Marshall Space Flight Center Launching the Future of Exploration and Science. Robert Lightfoot Acting Director July 29, 2009. Marshall’s Continuing Role in Space Exploration . Understanding Our World and Beyond. Living and Working In Space. Lifting from Earth.

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Cosmophysics Group KEK Theory Center 10-12 Nov. 2009

HEAP2009. High Energy Astrophysics 2009 - Cosmic Particles, Jets and Accelerator Science -. Cosmophysics Group KEK Theory Center 10-12 Nov. 2009. High Energy Astrophysics. A broad subject – stars, galaxies, BHs, etc. Cosmic Ray. Cosmic Jet. AGN. Microquasar. Pulsar. GRB.

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activities in KEK

activities in KEK. Takashi Sasaki. Japan Geant4 Users Group. Japanese discussion e-mail list almost 100 addresses help each other web pages http://www.geant4.org workshops December 2000 July 23-24, 2001 training June 2000. people joined the workshop. ATLAS JHF

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OSETI - Optical Search for Extra-terrestrial Intelligence

OSETI - Optical Search for Extra-terrestrial Intelligence Kristina Krylova : kkrylova@buffalo.edu, University at Buffalo – SUNY Dr . Corbin Covault : corbin.covault@cwru.edu, Case Western Reserve University. Abstract

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Simbol X: A New Generation Soft/Hard X-ray Telescope

Simbol X: A New Generation Soft/Hard X-ray Telescope. P. Slane, S. Romaine, S.S. Murray, R. Brissenden, M. Elvis, P.Gorenstein, E. Mattison, S. Steel (SAO), S. O’Dell, J. Kolodziejczak, B. Ramsey (NASA/MSFC), L. Angelini (NASA/GSFC), O. Citterio, G. Pareschi (Brera Observatory).

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