Table of contentsExploring the High Energy Universe where Particle Physics and Astrophysics Collide Mission GLAST Burst Monitor (GBM) Large Area Telescope (LAT) Pair Conversion Telescope LAT Schematic New Technologies EGRET vs. GLAST LAT EGRET’s Legacy EGRET All-Sky Map 3rd EGRET Catalog Simulated LAT all-sky map LAT Science Overview LAT Log N vs. Log S Unidentified Sources Possible Unidentified Sources EGRET Blazars Blazar questions/LAT Answers Slide 19 LAT studies 3C79 LAT studies EBL cutoff AGN Log N vs. Log S LAT vs. Ground-based HE Arrays Ground-based HET Arrays Multi-wavelength Mkn 501 Supernovae and Cosmic Rays LAT studies Supernova Remnants LAT studies SNR and CRs EGRET pulsars Outer gap vs. polar cap models Vela pulsar outer gap model LAT studies pulsars Slide 33 Dark Matter – a short review Searching for dark matter First Light from Dark Matter? Diffuse emission from Relic decay WIMP line detectability Conclusions For more information: Slide 41 LAT Studies Blazars |
Author: Lynn Cominsky E-mail: lynnc@charmian.sonoma.edu |