All Tables

Table 1: Afterglow detections for GRBs localised by recent $\gamma$ -ray missions between July 1996 and July 2007.
Table 2: GRBs detected by INTEGRAL. The columns refer to (from left to right): GRB; right ascension; declination; T₉₀ duration; peak flux; fluence; photon index; $\chi ^2$ /degrees of freedom (d.o.f.); afterglow detections in radio, R, infrared, IR, optical, O and X-ray, X. Peak fluxes, fluences and photon indices are given in the 20-200 keV energy range.
Table 3: IBIS and SPI spectral properties of GRBs for which Band and quasithermal (PL + BB) models are fit to spectra. Parameters quoted are low energy power-law index, $\alpha$ , high energy power-law index, $\beta$ , and break energy, E₀, for Band model fits and temperature, kT and power-law index, $\Gamma$ for quasithermal model fits.
Table 4: Spectral lag measurements for INTEGRAL GRBs. The columns refer to (from left to right): GRB; supergalactic longitude (SGL) and latitude (SGB); burst interval used in spectral lag determination relative to trigger time and as marked on time profiles in the Appendix; spectral lags measured between Channel 2 (50-100 keV) and Channel 1 (25-50 keV), $\tau _{2,1}$ , Channels 2 and 3 combined (50-300 keV) and Channel 1 (25-50 keV), $\tau _{2+3,1}$ and Channel 3 (100-300 keV) and Channel 1 (25-50 keV), $\tau _{3,1}$ .
Table 5: Wavelet-denoised spectral lags of weak GRBs. The lags derived from raw data are shown for comparison where available. Spectral lags measured between Channels 2 and 3 combined (50-300 keV) and Channel 1 (25-50 keV), $\tau _{2+3,1}$ , with the exception of the XRFs for which the lag is measured between 15-25 keV and 25-50 keV (Channel 1), $\tau _{1,15-25}$ .
Table 6: Median properties of the 28 long-duration GRBs with a measured $\tau _{2+3,1}$ , categorised into those with short lags ( $\tau_{2+3,1}<0.75~{\rm s}$ ) and long lags ( $\tau_{2+3,1}>0.75~{\rm s}$ .)