2009ApJ...696.2155G


Query : 2009ApJ...696.2155G

2009ApJ...696.2155G - Astrophys. J., 696, 2155-2169 (2009/May-2)

Broadband, time-dependent, spectroscopy of the brightest bursts observed by BATSE LAD and EGRET TASC.

GONZALEZ M.M., CARRILLO-BARRAGAN M., DINGUS B.L., KANEKO Y., PREECE R.D. and BRIGGS M.S.

Abstract (from CDS):

The Energetic Gamma Ray Experiment Telescope (EGRET) calorimeter, Total Absorption Shower Counter (TASC), was triggered by the Burst And Transient Source Experiment (BATSE) and thus observed several bursts in the energy range of 1-200 MeV. The analysis of combined BATSE Large Area Detector and EGRET TASC data have been developed and discussed previously. Spectroscopy of GRB941017 based on this analysis uncovered an MeV component that would be hidden in the brightness of the synchrotron component in a time-integrated spectrum of the whole burst, while separation into shorter time intervals allowed a unique identification of a new component different from the synchrotron component. In this paper the spectral temporal evolution of the 68 brightest long BATSE bursts, in the broadest energy range yet reported, is studied using the analysis used for GRB941017. We consider the Band function to describe the spectra from keV to MeV energies. Only 21 of the 68 bursts showed MeV emission detectable by TASC. We observed three bursts that contained spectra with peak energy Epeak>2 MeV.

Abstract Copyright:

Journal keyword(s): gamma rays: bursts - gamma rays: observations - methods: data analysis

Simbad objects: 21

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Number of rows : 21
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 3B 940217 gB 01 56.3 +04 33           ~ 204 0
2 GRB 970202 gB 03 14 -29.3           ~ 17 0
3 GRB 970411 gB 03 56 +34.3           ~ 15 0
4 3B 930506 gB 04 17.8 -05 58           ~ 32 0
5 GRB 980923 gB 05 07.8 -80 36           ~ 50 0
6 1B 910503 gB 05 49.8 +38 44           ~ 133 0
7 LP 321-30 PM* 08 33 21.4607296513 +23 00 11.690522680   18.8   16.7   ~ 34 0
8 GRB 990104 gB 08 38 +04.7           ~ 19 0
9 2B 920311 gB 08 39.0 -36 34           ~ 36 0
10 4B 970223 gB 09 38 +34.1           ~ 25 0
11 2B 920622 gB 10 48.4 +47 10           ~ 54 0
12 4B 950425 gB 10 52.6 -35 15           ~ 26 0
13 GRB 981203 gB 11 00 +32.0           ~ 14 0
14 GRB 990506 gB 11 54 41 -26 45.0           ~ 166 1
15 4B 940921 gB 13 39.6 -17 46           ~ 22 0
16 GRB 990728 gB 14 10 -58.4           ~ 12 0
17 GRB 990123 gB 15 25 29 +44 45.0     8.95     ~ 989 1
18 4B 941017 gB 20 06.2 +09 49           ~ 93 0
19 1B 910814 gB 23 05.4 +30 26           ~ 80 0
20 GRB 981021 gB 23 47 +01.0           ~ 14 0
21 GRB 970315 gB 23 48 +62.4           ~ 22 0

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