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Gamma-ray Astronomy. (The Short Story…). The Big Picture. Whole sky glows Extreme environments Probes of the Universe. CGRO/EGRET All Sky Map. Explorer 11. Early Gamma-ray Astronomy. • Gamma-ray Bursts Vela Program : A Bomb or Not a Bomb? A few hundred events, a few hundred theories
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Gamma-ray Astronomy (The Short Story…)
The Big Picture • Whole sky glows • Extreme environments • Probes of the Universe CGRO/EGRET All Sky Map
Early Gamma-ray Astronomy • • Gamma-ray Bursts • Vela Program : A Bomb or Not a Bomb? • A few hundred events, a few hundred theories • Gamma-ray Sources • SAS-2 – discovered 2 pulsars (1972) • COS-B – about 25 sources(1975-82) • Most unidentified, but 1 quasar • Diffuse extra-galactic background
Sources of g-ray Emission • Black holes • Active Galaxies • Pulsars •Gamma-ray bursts • Diffuse emission • Supernovae • Unidentified
CGRO/EGRET • Apr 1991 – Jun 2000 • 30 MeV – 30 GeV • 67%=5.85(100 MeV/E)0.534
The Third Egret Catalog E >100 MeV • EGRET cycles 1-4: 416 gamma-ray excesses above 3 sigma. • 271 of them included in the 3EG catalog. • The significance of sources close to the Galactic plane is 5 sigma. Sources off the the plane have 4 sigma.
High Energy Halo around Milky Way Courtesy of D. Dixon, University of California, Riverside
Gamma-ray Burst Progress • Beppo/SAX finds evidence for X-ray afterglow from several GRBs (2/28/97) • Jan van Paradijs finds optical afterglow • Redshifts indicate cosmological distances (Keck, HST) • ROTSE catches GRB in the act at visible wavelengths (1/23/99) • Evidence mounts for two types of GRBs
Models for GRBs Hypernova Merging Neutron Stars
New Missions = Better Data HETE II (launched 10/9/00) INTEGRAL (2002) Swift (2004) GLAST (2008) Swift
Gamma Ray Large Area Space Telescope • Launch in 2008? • 20 MeV to 300 GeV • Wide-field imaging telescope • NASA cost is $326
Gamma ray Air shower ~ 10 km ~ 1o Cherenkov light ~ 120 m Detection of TeV gamma rays with Cherenkov telescopes
New instruments coming online CANGAROO III H.E.S.S.
MAGIC VERITAS (photomontage)
Detection of TeV gamma rays from the Crab Nebula Whipple 1989: 50 h observation time HEGRA 1997: 15 min HESS 2004: 30 sec Progress
For More Information • Imagine the Universe! -http://imagine.gsfc.nasa.gov/ • Swift Mission - http://swift.sonoma.edu/ • GLAST Mission - http://ww-glast.sonoma.edu/ • CGRO Mission - http://cossc.gsfc.nasa.gov