1. Gamma-Ray Pulsars in the GLAST Era Gamma-ray Large Area Space Telescope Marcus Ziegler University of California Santa Cruz Bill Atwood Brian Baugmann Rober Johnson

2. GLAST basic principle Pair conversion telescope  e+e+ e–e– particle tracking detectors conversion foil Anticoincidence shield Pair-Conversion Telescope

3. GLAST status All detector components of the LAT (Large area Telescope) are assembled Tracker, Calorimeter, and Anti coincidence detector

4. Better PSF All detector components of the LAT (Large area Telescope) are assembled Tracker, Calorimeter, and Anti coincidence detector Simulated LAT (>1 GeV, 1 yr) Simulated LAT (>100 MeV, 1 yr)

5. Energy range All detector components of the LAT (Large area Telescope) are assembled Tracker, Calorimeter, and Anti coincidence detector

6. Different pulsar models Outer gap Polar cap Slot gap

7. Emission models All detector components of the LAT (Large area Telescope) are assembled Tracker, Calorimeter, and Anti coincidence detector

8. Source populstions All detector components of the LAT (Large area Telescope) are assembled Tracker, Calorimeter, and Anti coincidence detector

9. Search methods All detector components of the LAT (Large area Telescope) are assembled Tracker, Calorimeter, and Anti coincidence detector