INTSPIAGRB - INTEGRAL First SPI-ACS Gamma-Ray Burst Catalog
This table lists the properties of 388 GRB candidates detected from Oct 27, 2002 to Jan 15, 2005 with the Anti-Coincidence Shield (ACS) of SPI. It has numerous events with missing entries, notice. For all GRBs which were confirmed by other instruments but were detected by SPI-ACS below the sample selection threshold, only the time, date, significance and common instruments are listed. Furthermore, the variability measure was obtained only for long-duration events which had sufficiently large signal-to-noise ratios.
The 1st INTEGRAL SPI-ACS Gamma-Ray Burst Catalogue. Rau A., Kienlin A. von, Hurley K., Lichti G.G. <Astron. Astrophys. 438, 1175 (2005)> =2005A&A...438.1175R (SIMBAD/NED BibCode)
A unique identifying number for the event.
The event designation based on the date on which it occurred. The HEASARC has constructed this parameter by adding a 'GRB ' prefix to the YYMMDD date listed in the published table, and an 'a', 'b', etc., suffix if multiple GRBs occurred on the same day. Thus, the second burst which occurred on 2002 Nov 25 has been given the name of 'GRB 021125b'.
The trigger date and time in UTC, given to the nearest second.
The maximum significance of the event above the background, in terms of sigma.
The observer frame duration of the event, t_90, in seconds. This is the time interval over which the burst emitted from 5% to 95% of its total measured counts.
The uncertainty in the t_90 duration, in seconds.
The total integrated counts in the event, in kilocounts (kct).
The RMS uncertainty in the integrated counts, in kct.
The peak count rate over a 0.25 seconds interval, in kct/0.25s.
The RMS uncertainty in the peak count rate, in kct/0.25s.
The V/Vmax statistic for the event. V/Vmax compares the volume in which the event was detected to the largest possible volume in which the event would be just at the detection threshold. See the Schmidt M., 1968ApJ...151..393S for more details.
The variability measure for the event. The variability V(f=0.45) was computed from the variance of the 50 ms binned light curve with respect to a boxcar-smoothed version of itself following the formulation of Reichart et al. (2001ApJ...552...57R). A smoothing timescale of t_0.45, the effective time for which the integrated counts of the brightest part of the event comprise 45% of the total counts, was used.
The RMS uncertainty in the variability measure.
This parameter contains flags which identify all other gamma-ray instruments and missions for which detections of the event were reported. The designations of the other instruments are as follows:
U = Ulysses K = Konus/Wind M = Mars-Odyssey H = HETE-2 R = RHESSI C = Helicon/Coronas-F I = INTEGRAL (SPI/IBIS) S = Swift X = RXTE/ASM