All Tables
- Table 1:
Temporal properties of the pulses in GRB 040106.
- Table 2:
Spectral analysis results for GRB 040106 with SPI and IBIS/ISGRI for two intervals around the prominent peaks of emission. Errors quoted are for 1 parameter of interest at 1
confidence level. Fluxes are quoted for the energy range 20-200 keV. Within the large
errors on the spectral fits, results are consistent between instruments.
- Table 3:
Afterglow model tests using X-ray data. The condition for closure
depends on whether
or
(Col. 2). p is the power-law index of the emitting electron population.