Image Details
Caption: Fig. 1.
Swift light curves of GRB 041219a in (a) 25–50 keV, (b) 50–100 keV, and (c) 100–350 keV bands (Barthelmy et al. 2004), and the SPI light curves for the singles in the same bands in (d), (e), and (f), respectively. Times are relative to the peak of the precursor.
© 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.