grb_8121: 50-100 keV
grb_8121: 100-300 keV
grb_8121: >300 keV
grb_8116
grb_8113
(All figures above from http://www.batse.msfc.nasa.gov/batse/grb/lightcurve/)
Note different vertical axes!
X-ray afterglow spectrum from Swift (launched 2004).
GRB991208: Including host galaxy (upper curve)
GRB991208 and GRB990123
Evidence for supernova connection (only for long-soft?).
GRB990123: prompt optical emission reached 9th magnitude! (z=1.6!)
GRB (at least the long-soft ones) tend to occur in star-forming regions.
About 80 known.