A two-zone model for the production of prompt neutrinos in gamma-ray bursts Matías M. Reynoso IFIMAR-CONICET, Mar del Plata, Argentina GRACO 2, Buenos.
Masanori Ohno (ISAS/JAXA). HXD: 10-600 keV WAM: 50keV-5MeV XIS: 0.2-12keV X-ray Afterglow (XIS + HXD withToO) Wide energy band (0.2-600 keV) Ultra-low.
SONG Targets of Opportunity: Searching for Pulses in Gamma-Ray Burst Afterglows Jon Hakkila.
GRB Prompt Emission: Turbulence, Magnetic Field & Jitter Radiation Jirong Mao.
On some weaknesses of the standard afterglow model:
GRB
