The Fifth Compton Symposium: Portsmouth, NH, September 1999
Mark L. McConnell, James M. Ryan
American Inst. of Physics, Apr 20, 2000 - Science - 840 pages
With the Compton Gamma-Ray Observatory (CGRO) now in its ninth year of operation, the Fifth Compton Symposium provided an opportunity for sharing the most recent scientific results from CGRO and other related experiments in gamma-ray astronomy. Equally important were the descriptions of several new space-based and ground-based experiments in gamma-ray astronomy. These new instruments will be responsible for continuing the pioneering efforts of the CGRO mission. The proceedings provide a valuable reference for researchers in high energy astrophysics.
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GammaRay Line Astrophysics
Investigations of Positron Annihilation Radiation
TGRS Measurements of the Positron Annihilation Spectrum
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2000 American Institute acceleration accretion disk analysis angular resolution ASCA Astrophys Astrophysics background band BATSE BeppoSAX BL Lac objects black hole blazars bremsstrahlung burst CGRO COMPTEL Compton scattering continuum cosmic rays count rate Crab Cygnus density detected detector edited by M. L. EGRET EGRET sources electrons emission energy range field of view Fifth Compton Symposium FIGURE flare flux frequency Galaxy gamma gamma-ray GLAST hard X-ray heliostat high energy imaging Institute of Physics instrument INTEGRAL J. M. Ryan light curve Lorentz factor luminosity M. L. McConnell maps McConnell and J. M. measured mission monitoring neutron star novae observations Observatory optical orbital OSSE outbursts parameters particle peak phase photons point sources power law Proc pulsars pulse radiation radio redshift region RXTE sensitivity shows significant simulations solar spectrum supernova synchrotron telescope upper limits variability X-ray source