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.
Going out with a bang: HSTs continuing contribution to gamma-ray bursts Andrew Levan University of Warwick.
SGR activity in time Sergei Popov (SAI MSU) (HEA-2006, 25-27 December 2006 Moscow, IKI)
By: Courtney Lee & Kristel Curameng. Short-lived bursts of gamma-ray photons. Gamma-ray photons are the most energetic form of light. Some are associated.
Gamma-ray Bursts and Their Afterglows
Short GRBs and their Progenitors (in the era of pre-Gravitational Waves)
GRB (Gamma Ray Bursts) 17-05-2012 Tor Vergata. The Discovery The BATSE Era The prompt event era The Beppo-SAX Era The afterglow era The Swift Era The.
SONG Targets of Opportunity: Searching for Pulses in Gamma-Ray Burst Afterglows
MAGNETARS
Short-Duration Gamma-Ray Burst Central Engines
Refusing to Go Quietly: Gamma-Ray Bursts and Their Progenitors Andy Fruchter STScI Hubble Science Briefing 5 Dec. 2013.
V. V. Sokolov
