Targeting GRB events Swift now, Fermi (GLAST) keep looking at  rays from GRB. GRB powered by accretion disks on newly formed objects.
{"Image DocumentName": "Targeting GRB eventsSwift now, Fermi (GLAST) keep looking at \uf067 rays from GRB. GRB powered by accretion disks on newly formed objects.", "Image ImageDescription": "Neutrino and GW expected within a few ms delay. Short GRB (< 2s) potentially related to BNS, BH-NS. Long GRB (>2s, average 30s) related to (classes of) SNe. Again, boost detection confidence. Provide insight in the fireball mechanism.", "Image XResolution": "37", "Image YResolution": "37", "Image ResolutionUnit": "Pixels/Centimeter", "Image Software": "SlidePlayer", "Image YCbCrPositioning": "Centered"}