grb_8121: 20-50 keV
grb_8121: 50-100 keV
grb_8121: 100-300 keV
grb_8121: >300 keV
grb_8120
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.