1999ApJ...519..206C


Query : 1999ApJ...519..206C

1999ApJ...519..206C - Astrophys. J., 519, 206-213 (1999/July-1)

Spectral hardness decay with respect to fluence in BATSE gamma-ray bursts.

CRIDER A., LIANG E.P., PREECE R.D., BRIGGS M.S., PENDLETON G.N., PACIESAS W.S., BAND D.L. and MATTESON J.L.

Abstract (from CDS):

We have analyzed the evolution of the spectral hardness parameter Epk (the maximum of the νFν spectrum) as a function of fluence in gamma-ray bursts. We fit 41 pulses within 26 bursts with the trend reported by Liang & Kargatis, which found that Epk decays exponentially with respect to photon fluence Φ(t). We also fit these pulses with a slight modification of this trend, where Epk decays linearly with energy fluence. In both cases, we found the set of 41 pulses to be consistent with the trend. For the latter trend, which we believe to be more physical, the distribution of the decay constant Φ0 is roughly lognormal, where the mean of log10 Φ0 is 1.75±0.07 and the FWHM of log10 Φ0 is 1.0±0.1. Regarding an earlier reported invariance in Φ0 among different pulses in a single burst, we found probabilities of 0.49-0.84 (depending on the test used) that such invariance would occur by coincidence, most likely because of the narrow distribution of Φ0 values among pulses.

Abstract Copyright: ∼

Journal keyword(s): Gamma Rays: Bursts - Gamma Rays: Observations

Simbad objects: 26

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Number of rows : 26
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 3B 930425B gB 01 12.0 -35 11           ~ 20 0
2 4B 950111B gB 01 15.9 -11 26           ~ 13 0
3 4B 941121 gB 02 21.8 -66 22           ~ 21 0
4 4B 951016 gB 02 23.3 -24 22           ~ 25 0
5 GRB 950403B gB 02 25.6 +10 43           ~ 20 0
6 GRB 961001 gB 02 31 +59.4           ~ 20 0
7 3B 931026 gB 03 25.4 -10 34           ~ 17 0
8 GRB 950325A gB 04 24.9 -11 34           ~ 19 0
9 3B 940623 gB 07 13.5 +75 47           ~ 25 0
10 2B 921015 gB 08 12.2 +41 41           ~ 25 0
11 2B 921003 gB 10 01.3 -14 43           ~ 23 0
12 1B 910807 gB 10 15.4 +06 29           ~ 38 0
13 4B 960807 gB 10 30.1 +32 08           ~ 21 0
14 1B 911118 gB 11 08.1 -20 51           ~ 61 0
15 1B 910627 gB 13 12.0 -02 29           ~ 54 0
16 4B 940921 gB 13 39.6 -17 46           ~ 22 0
17 GRB 940529C gB 14 19.4 +58 56           ~ 34 0
18 4B 960114 gB 14 24.8 -29 44           ~ 23 0
19 GRB 970111 gB 15 28 15.0 +19 36 18           ~ 140 0
20 1B 910717 gB 16 39.4 -58 13           ~ 41 0
21 2B 930120 gB 17 25.2 +14 44           ~ 37 0
22 3B 930922 gB 18 04.8 +55 53           ~ 23 0
23 1B 911031 gB 18 58.2 +21 20           ~ 45 0
24 2B 920718 gB 19 45.6 -55 59           ~ 36 0
25 4B 941008 gB 20 22.5 -52 11           ~ 16 0
26 2B 921207 gB 20 25.3 -42 56           ~ 47 0

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